Search results for: +Astronomy and astrophysics, page 1 | Collections Search Center, Smithsonian Institution

The Earliest Galaxies: Exploring Cosmic Sunrise with Hubble, Spitzer, and JWST

Creator:: National Air and Space Museum Search this

Type:: Lectures; YouTube Videos

Uploaded:: 2018-03-22T22:00:10.000Z

YouTube Category:: Education Search this

Topic:: Aeronautics;Flight;Space Sciences Search this

See more by:: airandspace

Data Source:: National Air and Space Museum

YouTube Channel:: airandspace

EDAN-URL:: edanmdm:yt_MTgqlzEoaB8

Behind the Scenes with Project PHaEDRA: How the Notebooks Were Used in Research

Creator:: Smithsonian Institution Search this

Type:: YouTube Videos

Uploaded:: 2018-10-19T14:36:48.000Z

YouTube Category:: Education Search this

Topic:: Transcription Search this

See more by:: SmithsonianTranscription

Data Source:: Smithsonian Institution

YouTube Channel:: SmithsonianTranscription

EDAN-URL:: edanmdm:yt_rXv8KANr798

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Differences in physical properties of coronal bright points and their ALMA counterparts within and outside coronal holes

Author:: Matković, F. Search this; Brajša, R. Search this; Temmer, M. Search this; Heinemann, S. G. Search this; Ludwig, H. -G Search this; Saar, S. H. Search this; Selhorst, C. L. Search this; Skokić, I. Search this; Sudar, D. Search this

Object Type:: Smithsonian staff publication

Year:: 2023

Citation:: Matković, F., Brajša, R., Temmer, M., Heinemann, S. G., Ludwig, H. -G, Saar, S. H., Selhorst, C. L., Skokić, I., and Sudar, D. 2023. "Differences in physical properties of coronal bright points and their ALMA counterparts within and outside coronal holes." Astronomy and Astrophysics, 670 A146. https://doi.org/10.1051/0004-6361/202244160.

Identifier:: 168272

DOI:: https://doi.org/10.1051/0004-6361/202244160

ISSN:: 0004-6361

Data source:: Smithsonian Libraries and Archives

EDAN-URL:: edanmdm:slasro_168272

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An empirical model of the Gaia DR3 selection function

Author:: Cantat-Gaudin, Tristan Search this; Fouesneau, Morgan Search this; Rix, Hans-Walter Search this; Brown, Anthony G. A. Search this; Castro-Ginard, Alfred Search this; Kostrzewa-Rutkowska, Zuzanna Search this; Drimmel, Ronald Search this; Hogg, David W. Search this; Casey, Andrew R. Search this; Khanna, Shourya Search this; Oh, Semyeong Search this; Price-Whelan, Adrian M. Search this; Belokurov, Vasily Search this; Saydjari, Andrew K. Search this; Green, G. Search this

Object Type:: Smithsonian staff publication

Year:: 2023

Citation:: Cantat-Gaudin, Tristan, Fouesneau, Morgan, Rix, Hans-Walter, Brown, Anthony G. A., Castro-Ginard, Alfred, Kostrzewa-Rutkowska, Zuzanna, Drimmel, Ronald, Hogg, David W., Casey, Andrew R., Khanna, Shourya, Oh, Semyeong, Price-Whelan, Adrian M., Belokurov, Vasily, Saydjari, Andrew K., and Green, G. 2023. "An empirical model of the Gaia DR3 selection function." Astronomy and Astrophysics, 669 A55. https://doi.org/10.1051/0004-6361/202244784.

Identifier:: 168279

DOI:: https://doi.org/10.1051/0004-6361/202244784

ISSN:: 0004-6361

Data source:: Smithsonian Libraries and Archives

EDAN-URL:: edanmdm:slasro_168279

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High-resolution X-ray spectra of RS Ophiuchi (2006 and 2021): Revealing the cause of SSS variability

Author:: Ness, J. -U Search this; Beardmore, A. P. Search this; Bode, M. F. Search this; Darnley, M. J. Search this; Dobrotka, A. Search this; Drake, J. J. Search this; Magdolen, J. Search this; Munari, U. Search this; Osborne, J. P. Search this; Orio, M. Search this; Page, K. L. Search this; Starrfield, S. Search this

Object Type:: Smithsonian staff publication

Year:: 2023

Citation:: Ness, J. -U, Beardmore, A. P., Bode, M. F., Darnley, M. J., Dobrotka, A., Drake, J. J., Magdolen, J., Munari, U., Osborne, J. P., Orio, M., Page, K. L., and Starrfield, S. 2023. "High-resolution X-ray spectra of RS Ophiuchi (2006 and 2021): Revealing the cause of SSS variability." Astronomy and Astrophysics, 670 A131. https://doi.org/10.1051/0004-6361/202245269.

Identifier:: 168281

DOI:: https://doi.org/10.1051/0004-6361/202245269

ISSN:: 0004-6361

Data source:: Smithsonian Libraries and Archives

EDAN-URL:: edanmdm:slasro_168281

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Understanding star formation in molecular clouds. IV. Column density PDFs from quiescent to massive molecular clouds

Author:: Schneider, N. Search this; Ossenkopf-Okada, V. Search this; Clarke, S. Search this; Klessen, R. S. Search this; Kabanovic, S. Search this; Veltchev, T. Search this; Bontemps, S. Search this; Dib, S. Search this; Csengeri, T. Search this; Federrath, C. Search this; Di Francesco, J. Search this; Motte, F. Search this; André, Ph Search this; Arzoumanian, D. Search this; Beattie, J. R. Search this; Bonne, L. Search this; Didelon, P. Search this; Elia, D. Search this; Könyves, V. Search this; Kritsuk, A. Search this; Ladjelate, B. Search this; Myers, Philip Search this; Pezzuto, S. Search this; Robitaille, J. F. Search this; Roy, A. Search this; Seifried, D. Search this; Simon, R. Search this; Soler, J. Search this; Ward-Thompson, D. Search this

Object Type:: Smithsonian staff publication

Year:: 2022

Citation:: Schneider, N., Ossenkopf-Okada, V., Clarke, S., Klessen, R. S., Kabanovic, S., Veltchev, T., Bontemps, S., Dib, S., Csengeri, T., Federrath, C., Di Francesco, J., Motte, F., André, Ph, Arzoumanian, D., Beattie, J. R., Bonne, L., Didelon, P., Elia, D., Könyves, V., Kritsuk, A., Ladjelate, B., Myers, Philip, Pezzuto, S., Robitaille, J. F., Roy, A. et al. 2022. "Understanding star formation in molecular clouds. IV. Column density PDFs from quiescent to massive molecular clouds." Astronomy and Astrophysics, 666 A165. https://doi.org/10.1051/0004-6361/202039610.

Identifier:: 168287

DOI:: https://doi.org/10.1051/0004-6361/202039610

ISSN:: 0004-6361

Data source:: Smithsonian Libraries and Archives

EDAN-URL:: edanmdm:slasro_168287

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Kinematics and brightness temperatures of transition discs. A survey of gas substructures as seen with ALMA

Author:: Wölfer, L. Search this; Facchini, S. Search this; van der Marel, N. Search this; van Dishoeck, E. F. Search this; Benisty, M. Search this; Bohn, A. J. Search this; Francis, L. Search this; Izquierdo, A. F. Search this; Teague, R. D. Search this

Object Type:: Smithsonian staff publication

Year:: 2023

Citation:: Wölfer, L., Facchini, S., van der Marel, N., van Dishoeck, E. F., Benisty, M., Bohn, A. J., Francis, L., Izquierdo, A. F., and Teague, R. D. 2023. "Kinematics and brightness temperatures of transition discs. A survey of gas substructures as seen with ALMA." Astronomy and Astrophysics, 670 A154. https://doi.org/10.1051/0004-6361/202243601.

Identifier:: 168289

DOI:: https://doi.org/10.1051/0004-6361/202243601

ISSN:: 0004-6361

Data source:: Smithsonian Libraries and Archives

EDAN-URL:: edanmdm:slasro_168289

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The GAPS programme at TNG. XL. A puffy and warm Neptune-sized planet and an outer Neptune-mass candidate orbiting the solar-type star TOI-1422

Author:: Naponiello, L. Search this; Mancini, L. Search this; Damasso, M. Search this; Bonomo, A. S. Search this; Sozzetti, A. Search this; Nardiello, D. Search this; Biazzo, K. Search this; Stognone, R. G. Search this; Lillo-Box, J. Search this; Lanza, A. F. Search this; Poretti, E. Search this; Lissauer, J. J. Search this; Zeng, L. Search this; Bieryla, A. Search this; Hébrard, G. Search this; Basilicata, M. Search this; Benatti, S. Search this; Bignamini, A. Search this; Borsa, F. Search this; Claudi, R. Search this; Cosentino, R. Search this; Covino, E. Search this; de Gurtubai, A. Search this; Delfosse, X. Search this; Desidera, S. Search this; Dragomir, D. Search this; Eastman, J. D. Search this; Essack, Z. Search this; Fiorenzano, A. F. M. Search this; Giacobbe, P. Search this; Harutyunyan, A. Search this; Heidari, N. Search this; Hellier, C. Search this; Jenkins, J. M. Search this; Knapic, C. Search this; König, P. -C Search this; Latham, D. W. Search this; Magazzù, A. Search this; Maggio, A. Search this; Maldonado, J. Search this; Micela, G. Search this; Molinari, E. Search this; Molinaro, M. Search this; Morgan, E. H. Search this; Moutou, C. Search this; Nascimbeni, V. Search this; Pace, E. Search this; Pagano, I. Search this; Pedani, M. Search this; Piotto, G. Search this; Pinamonti, M. Search this; Quintana, E. V. Search this; Rainer, M. Search this; Ricker, G. R. Search this; Seager, S. Search this; Twicken, J. D. Search this; Vanderspek, R. Search this; Winn, J. N. Search this

Object Type:: Smithsonian staff publication

Year:: 2022

Citation:: Naponiello, L., Mancini, L., Damasso, M., Bonomo, A. S., Sozzetti, A., Nardiello, D., Biazzo, K., Stognone, R. G., Lillo-Box, J., Lanza, A. F., Poretti, E., Lissauer, J. J., Zeng, L., Bieryla, A., Hébrard, G., Basilicata, M., Benatti, S., Bignamini, A., Borsa, F., Claudi, R., Cosentino, R., Covino, E., de Gurtubai, A., Delfosse, X., Desidera, S. et al. 2022. "The GAPS programme at TNG. XL. A puffy and warm Neptune-sized planet and an outer Neptune-mass candidate orbiting the solar-type star TOI-1422." Astronomy and Astrophysics, 667 A8. https://doi.org/10.1051/0004-6361/202244079.

Identifier:: 168316

DOI:: https://doi.org/10.1051/0004-6361/202244079

ISSN:: 0004-6361

Data source:: Smithsonian Libraries and Archives

EDAN-URL:: edanmdm:slasro_168316

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A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N

Author:: König, P. -C Search this; Damasso, M. Search this; Hébrard, G. Search this; Naponiello, L. Search this; Cortés-Zuleta, P. Search this; Biazzo, K. Search this; Santos, N. C. Search this; Bonomo, A. S. Search this; Lecavelier des Étangs, A. Search this; Zeng, L. Search this; Hoyer, S. Search this; Sozzetti, A. Search this; Affer, L. Search this; Almenara, J. M. Search this; Benatti, S. Search this; Bieryla, A. Search this; Boisse, I. Search this; Bonfils, X. Search this; Boschin, W. Search this; Carmona, A. Search this; Claudi, R. Search this; Collins, K. A. Search this; Dalal, S. Search this; Deleuil, M. Search this; Delfosse, X. Search this; Demangeon, O. D. S. Search this; Desidera, S. Search this; Díaz, R. F. Search this; Forveille, T. Search this; Heidari, N. Search this; Hussain, G. A. J. Search this; Jenkins, J. Search this; Kiefer, F. Search this; Lacedelli, G. Search this; Latham, D. W. Search this; Malavolta, L. Search this; Mancini, L. Search this; Martioli, E. Search this; Micela, G. Search this; Miles-Páez, P. A. Search this; Moutou, C. Search this; Nardiello, D. Search this; Nascimbeni, V. Search this; Pinamonti, M. Search this; Piotto, G. Search this; Ricker, G. Search this; Schwarz, R. P. Search this; Seager, S. Search this; Stognone, R. G. Search this; Strøm, P. A. Search this; Vanderspek, R. Search this; Winn, J. Search this; Wittrock, J. Search this

Object Type:: Smithsonian staff publication

Year:: 2022

Citation:: König, P. -C, Damasso, M., Hébrard, G., Naponiello, L., Cortés-Zuleta, P., Biazzo, K., Santos, N. C., Bonomo, A. S., Lecavelier des Étangs, A., Zeng, L., Hoyer, S., Sozzetti, A., Affer, L., Almenara, J. M., Benatti, S., Bieryla, A., Boisse, I., Bonfils, X., Boschin, W., Carmona, A., Claudi, R., Collins, K. A., Dalal, S., Deleuil, M., Delfosse, X. et al. 2022. "A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N." Astronomy and Astrophysics, 666 A183. https://doi.org/10.1051/0004-6361/202143002.

Identifier:: 168318

DOI:: https://doi.org/10.1051/0004-6361/202143002

ISSN:: 0004-6361

Data source:: Smithsonian Libraries and Archives

EDAN-URL:: edanmdm:slasro_168318

No Image Available

Gaia-TESS synergy: improving the identification of transit candidates

Author:: Panahi, Aviad Search this; Mazeh, Tsevi Search this; Zucker, Shay Search this; Latham, David W. Search this; Collins, Karen A. Search this; Rimoldini, Lorenzo Search this; Evans, Dafydd Wyn Search this; Eyer, Laurent Search this

Object Type:: Smithsonian staff publication

Year:: 2022

Citation:: Panahi, Aviad, Mazeh, Tsevi, Zucker, Shay, Latham, David W., Collins, Karen A., Rimoldini, Lorenzo, Evans, Dafydd Wyn, and Eyer, Laurent. 2022. "Gaia-TESS synergy: improving the identification of transit candidates." Astronomy and Astrophysics, 667 A14. https://doi.org/10.1051/0004-6361/202244207.

Identifier:: 168319

DOI:: https://doi.org/10.1051/0004-6361/202244207

ISSN:: 0004-6361

Data source:: Smithsonian Libraries and Archives

EDAN-URL:: edanmdm:slasro_168319

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TOI-3884 b: A rare 6-RE planet that transits a low-mass star with a giant and likely polar spot

Author:: Almenara, J. M. Search this; Bonfils, X. Search this; Forveille, T. Search this; Astudillo-Defru, N. Search this; Ciardi, D. R. Search this; Schwarz, R. P. Search this; Collins, K. A. Search this; Cointepas, M. Search this; Lund, M. B. Search this; Bouchy, F. Search this; Charbonneau, D. Search this; Díaz, R. F. Search this; Delfosse, X. Search this; Kidwell, R. C. Search this; Kunimoto, M. Search this; Latham, D. W. Search this; Lissauer, J. J. Search this; Murgas, F. Search this; Ricker, G. Search this; Seager, S. Search this; Vezie, M. Search this; Watanabe, D. Search this

Object Type:: Smithsonian staff publication

Year:: 2022

Citation:: Almenara, J. M., Bonfils, X., Forveille, T., Astudillo-Defru, N., Ciardi, D. R., Schwarz, R. P., Collins, K. A., Cointepas, M., Lund, M. B., Bouchy, F., Charbonneau, D., Díaz, R. F., Delfosse, X., Kidwell, R. C., Kunimoto, M., Latham, D. W., Lissauer, J. J., Murgas, F., Ricker, G., Seager, S., Vezie, M., and Watanabe, D. 2022. "TOI-3884 b: A rare 6-R_E planet that transits a low-mass star with a giant and likely polar spot." Astronomy and Astrophysics, 667 L11. https://doi.org/10.1051/0004-6361/202244791.

Identifier:: 168320

DOI:: https://doi.org/10.1051/0004-6361/202244791

ISSN:: 0004-6361

Data source:: Smithsonian Libraries and Archives

EDAN-URL:: edanmdm:slasro_168320

No Image Available

Constraining planetary mass-loss rates by simulating Parker wind profiles with Cloudy

Author:: Linssen, D. C. Search this; Oklopčić, A. Search this; MacLeod, Morgan Search this

Object Type:: Smithsonian staff publication

Year:: 2022

Citation:: Linssen, D. C., Oklopčić, A., and MacLeod, Morgan. 2022. "Constraining planetary mass-loss rates by simulating Parker wind profiles with Cloudy." Astronomy and Astrophysics, 667 A54. https://doi.org/10.1051/0004-6361/202243830.

Identifier:: 168330

DOI:: https://doi.org/10.1051/0004-6361/202243830

ISSN:: 0004-6361

Data source:: Smithsonian Libraries and Archives

EDAN-URL:: edanmdm:slasro_168330

No Image Available

Deep low-frequency radio observations of Abell 2256. II. The ultra-steep spectrum radio halo

Author:: Rajpurohit, K. Search this; Osinga, E. Search this; Brienza, M. Search this; Botteon, A. Search this; Brunetti, G. Search this; Forman, W. R. Search this; Riseley, C. J. Search this; Vazza, F. Search this; Bonafede, A. Search this; van Weeren, R. J. Search this; Brüggen, M. Search this; Rajpurohit, S. Search this; Drabent, A. Search this; Dallacasa, D. Search this; Rossetti, M. Search this; Rajpurohit, A. S. Search this; Hoeft, M. Search this; Bonnassieux, E. Search this; Cassano, R. Search this; Miley, G. K. Search this

Object Type:: Smithsonian staff publication

Year:: 2023

Citation:: Rajpurohit, K., Osinga, E., Brienza, M., Botteon, A., Brunetti, G., Forman, W. R., Riseley, C. J., Vazza, F., Bonafede, A., van Weeren, R. J., Brüggen, M., Rajpurohit, S., Drabent, A., Dallacasa, D., Rossetti, M., Rajpurohit, A. S., Hoeft, M., Bonnassieux, E., Cassano, R., and Miley, G. K. 2023. "Deep low-frequency radio observations of Abell 2256. II. The ultra-steep spectrum radio halo." Astronomy and Astrophysics, 669 A1. https://doi.org/10.1051/0004-6361/202244925.

Identifier:: 168347

DOI:: https://doi.org/10.1051/0004-6361/202244925

ISSN:: 0004-6361

Data source:: Smithsonian Libraries and Archives

EDAN-URL:: edanmdm:slasro_168347

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The origin of double-peak emission-line galaxies: Rotating discs, bars, or galaxy mergers?

Author:: Maschmann, Daniel Search this; Halle, Anaëlle Search this; Melchior, Anne-Laure Search this; Combes, Françoise Search this; Chilingarian, Igor V. Search this

Object Type:: Smithsonian staff publication

Year:: 2023

Citation:: Maschmann, Daniel, Halle, Anaëlle, Melchior, Anne-Laure, Combes, Françoise, and Chilingarian, Igor V. 2023. "The origin of double-peak emission-line galaxies: Rotating discs, bars, or galaxy mergers?" Astronomy and Astrophysics, 670 A46. https://doi.org/10.1051/0004-6361/202244746.

Identifier:: 168368

DOI:: https://doi.org/10.1051/0004-6361/202244746

ISSN:: 0004-6361

Data source:: Smithsonian Libraries and Archives

EDAN-URL:: edanmdm:slasro_168368

No Image Available

Gas condensation in brightest group galaxies unveiled with MUSE. Morphology and kinematics of the ionized gas

Author:: Olivares, V. Search this; Salomé, P. Search this; Hamer, S. L. Search this; Combes, F. Search this; Gaspari, M. Search this; Kolokythas, K. Search this; O'Sullivan, Ewan Search this; Beckmann, R. S. Search this; Babul, A. Search this; Polles, F. L. Search this; Lehnert, M. Search this; Loubser, S. I. Search this; Donahue, M. Search this; Gendron-Marsolais, M. -L Search this; Lagos, P. Search this; Pineau des Forets, G. Search this; Godard, B. Search this; Rose, T. Search this; Tremblay, Grant Search this; Ferland, G. Search this; Guillard, P. Search this

Object Type:: Smithsonian staff publication

Year:: 2022

Citation:: Olivares, V., Salomé, P., Hamer, S. L., Combes, F., Gaspari, M., Kolokythas, K., O'Sullivan, Ewan, Beckmann, R. S., Babul, A., Polles, F. L., Lehnert, M., Loubser, S. I., Donahue, M., Gendron-Marsolais, M. -L, Lagos, P., Pineau des Forets, G., Godard, B., Rose, T., Tremblay, Grant, Ferland, G., and Guillard, P. 2022. "Gas condensation in brightest group galaxies unveiled with MUSE. Morphology and kinematics of the ionized gas." Astronomy and Astrophysics, 666 A94. https://doi.org/10.1051/0004-6361/202142475.

Identifier:: 168372

DOI:: https://doi.org/10.1051/0004-6361/202142475

ISSN:: 0004-6361

Data source:: Smithsonian Libraries and Archives

EDAN-URL:: edanmdm:slasro_168372

No Image Available

Gas kinematics around filamentary structures in the Orion B cloud

Author:: Gaudel, Mathilde Search this; Orkisz, Jan H. Search this; Gerin, Maryvonne Search this; Pety, Jérôme Search this; Roueff, Antoine Search this; Marchal, Antoine Search this; Levrier, François Search this; Miville-Deschênes, Marc-Antoine Search this; Goicoechea, Javier R. Search this; Roueff, Evelyne Search this; Le Petit, Franck Search this; de Souza Magalhaes, Victor Search this; Palud, Pierre Search this; Santa-Maria, Miriam G. Search this; Vono, Maxime Search this; Bardeau, Sébastien Search this; Bron, Emeric Search this; Chainais, Pierre Search this; Chanussot, Jocelyn Search this; Gratier, Pierre Search this; Guzman, Viviana Search this; Hughes, Annie Search this; Kainulainen, Jouni Search this; Languignon, David Search this; Le Bourlot, Jacques Search this; Liszt, Harvey Search this; Öberg, Karin Search this; Peretto, Nicolas Search this; Sievers, Albrecht Search this; Tremblin, Pascal Search this

Object Type:: Smithsonian staff publication

Year:: 2023

Citation:: Gaudel, Mathilde, Orkisz, Jan H., Gerin, Maryvonne, Pety, Jérôme, Roueff, Antoine, Marchal, Antoine, Levrier, François, Miville-Deschênes, Marc-Antoine, Goicoechea, Javier R., Roueff, Evelyne, Le Petit, Franck, de Souza Magalhaes, Victor, Palud, Pierre, Santa-Maria, Miriam G., Vono, Maxime, Bardeau, Sébastien, Bron, Emeric, Chainais, Pierre, Chanussot, Jocelyn, Gratier, Pierre, Guzman, Viviana, Hughes, Annie, Kainulainen, Jouni, Languignon, David, Le Bourlot, Jacques et al. 2023. "Gas kinematics around filamentary structures in the Orion B cloud." Astronomy and Astrophysics, 670 A59. https://doi.org/10.1051/0004-6361/202142109.

Identifier:: 168394

DOI:: https://doi.org/10.1051/0004-6361/202142109

ISSN:: 0004-6361

Data source:: Smithsonian Libraries and Archives

EDAN-URL:: edanmdm:slasro_168394

No Image Available

Gas phase Elemental abundances in Molecular cloudS (GEMS). VII. Sulfur elemental abundance

Author:: Fuente, A. Search this; Rivière-Marichalar, P. Search this; Beitia-Antero, L. Search this; Caselli, P. Search this; Wakelam, V. Search this; Esplugues, G. Search this; Rodríguez-Baras, M. Search this; Navarro-Almaida, D. Search this; Gerin, M. Search this; Kramer, C. Search this; Bachiller, R. Search this; Goicoechea, J. R. Search this; Jiménez-Serra, I. Search this; Loison, J. C. Search this; Ivlev, A. Search this; Martín-Doménech, R. Search this; Spezzano, S. Search this; Roncero, O. Search this; Muñoz-Caro, G. Search this; Cazaux, S. Search this; Marcelino, N. Search this

Object Type:: Smithsonian staff publication

Year:: 2023

Citation:: Fuente, A., Rivière-Marichalar, P., Beitia-Antero, L., Caselli, P., Wakelam, V., Esplugues, G., Rodríguez-Baras, M., Navarro-Almaida, D., Gerin, M., Kramer, C., Bachiller, R., Goicoechea, J. R., Jiménez-Serra, I., Loison, J. C., Ivlev, A., Martín-Doménech, R., Spezzano, S., Roncero, O., Muñoz-Caro, G., Cazaux, S., and Marcelino, N. 2023. "Gas phase Elemental abundances in Molecular cloudS (GEMS). VII. Sulfur elemental abundance." Astronomy and Astrophysics, 670 A114. https://doi.org/10.1051/0004-6361/202244843.

Identifier:: 168504

DOI:: https://doi.org/10.1051/0004-6361/202244843

ISSN:: 0004-6361

Data source:: Smithsonian Libraries and Archives

EDAN-URL:: edanmdm:slasro_168504

No Image Available

Magnetically regulated collapse in the B335 protostar?. II. Observational constraints on gas ionization and magnetic field coupling

Author:: Cabedo, Victoria Search this; Maury, Anaëlle Search this; Girart, Josep Miquel Search this; Padovani, Marco Search this; Hennebelle, Patrick Search this; Houde, Martin Search this; Zhang, Qizhou Search this

Object Type:: Smithsonian staff publication

Year:: 2023

Citation:: Cabedo, Victoria, Maury, Anaëlle, Girart, Josep Miquel, Padovani, Marco, Hennebelle, Patrick, Houde, Martin, and Zhang, Qizhou. 2023. "Magnetically regulated collapse in the B335 protostar?. II. Observational constraints on gas ionization and magnetic field coupling." Astronomy and Astrophysics, 669 A90. https://doi.org/10.1051/0004-6361/202243813.

Identifier:: 168522

DOI:: https://doi.org/10.1051/0004-6361/202243813

ISSN:: 0004-6361

Data source:: Smithsonian Libraries and Archives

EDAN-URL:: edanmdm:slasro_168522

No Image Available

Galaxy populations in the most distant SPT-SZ clusters. II. Galaxy structural properties in massive clusters at 1.4 ≲ z ≲ 1.7

Author:: Strazzullo, V. Search this; Pannella, M. Search this; Mohr, J. J. Search this; Saro, A. Search this; Ashby, M. L. N. Search this; Bayliss, M. B. Search this; Canning, R. E. A. Search this; Floyd, B. Search this; Gonzalez, A. H. Search this; Khullar, G. Search this; Kim, K. J. Search this; McDonald, M. Search this; Reichardt, C. L. Search this; Sharon, K. Search this; Somboonpanyakul, T. Search this

Object Type:: Smithsonian staff publication

Year:: 2023

Citation:: Strazzullo, V., Pannella, M., Mohr, J. J., Saro, A., Ashby, M. L. N., Bayliss, M. B., Canning, R. E. A., Floyd, B., Gonzalez, A. H., Khullar, G., Kim, K. J., McDonald, M., Reichardt, C. L., Sharon, K., and Somboonpanyakul, T. 2023. "Galaxy populations in the most distant SPT-SZ clusters. II. Galaxy structural properties in massive clusters at 1.4 ≲ z ≲ 1.7." Astronomy and Astrophysics, 669 A131. https://doi.org/10.1051/0004-6361/202245268.

Identifier:: 168535

DOI:: https://doi.org/10.1051/0004-6361/202245268

ISSN:: 0004-6361

Data source:: Smithsonian Libraries and Archives

EDAN-URL:: edanmdm:slasro_168535

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i(cm)z, a semi-analytic model for the thermodynamic properties in galaxy clusters: Calibrations with mass and redshift, and implication for the hydrostatic bias

Author:: Ettori, S. Search this; Lovisari, L. Search this; Eckert, D. Search this

Object Type:: Smithsonian staff publication

Year:: 2023

Citation:: Ettori, S., Lovisari, L., and Eckert, D. 2023. "i(cm)z, a semi-analytic model for the thermodynamic properties in galaxy clusters: Calibrations with mass and redshift, and implication for the hydrostatic bias." Astronomy and Astrophysics, 669 A133. https://doi.org/10.1051/0004-6361/202245002.

Identifier:: 168536

DOI:: https://doi.org/10.1051/0004-6361/202245002

ISSN:: 0004-6361

Data source:: Smithsonian Libraries and Archives

EDAN-URL:: edanmdm:slasro_168536

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i(cm)z, a semi-analytic model for the thermodynamic properties in galaxy clusters: Calibrations with mass and redshift, and implication for the hydrostatic bias

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