The VLT/SPHERE view of the ATOMIUM cool evolved star sample I. Overview: Sample characterization through polarization analysis

Autor: M. Montargès, E. Cannon, A. de Koter, T. Khouri, E. Lagadec, P. Kervella, L. Decin, I. McDonald, W. Homan, L. B. F. M. Waters, R. Sahai, C. A. Gottlieb, J. Malfait, S. Maes, B. Pimpanuwat, M. Jeste, T. Danilovich, F. De Ceuster, M. Van de Sande, D. Gobrecht, S. H. J. Wallström, K. T. Wong, I. El Mellah, J. Bolte, F. Herpin, A. M. S. Richards, A. Baudry, S. Etoka, M. D. Gray, T. J. Millar, K. M. Menten, H. S. P. Müller, J. M. C. Plane, J. Yates, A. Zijlstra

Publikováno v: Montargès, M, Cannon, E, Koter, A D, Khouri, T, Lagadec, E, Kervella, P, Decin, L, McDonald, I, Homan, W, Waters, L B F M, Sahai, R, Gottlieb, C A, Malfait, J, Maes, S, Pimpanuwat, B, Jeste, M, Danilovich, T, Ceuster, F D, Sande, M V D, Gobrecht, D, Wallström, S H J, Wong, K T, Mellah, I E, Bolte, J, Herpin, F, Richards, A M S, Baudry, A, Etoka, S, Gray, M D, Millar, T J, Menten, K M, Müller, H S P, Plane, J M C, Yates, J & Zijlstra, A 2023, ' The VLT/SPHERE view of the ATOMIUM cool evolved star sample: I. Overview: sample characterization through polarization analysis ', Astronomy and Astrophysics, vol. 671, A96 . https://doi.org/10.1051/0004-6361/202245398
Astronomy & Astrophysics, 671, pp. 1-22
Astronomy & Astrophysics, 671, 1-22

Aims. Through the ATOMIUM project, based on an ALMA large program, we aim to present a consistent view of a sample of 17 nearby cool evolved stars (Aymptotic Giant Branch and red supergiant stars). Methods. Here we present VLT/SPHERE-ZIMPOL polarimet

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4fe89cd5b1452752863127a50cb36a41
https://hdl.handle.net/2066/291694

The sharp ALMA view of infall and outflow in the massive protocluster G31.41+0.31

Autor: M. T. Beltrán, V. M. Rivilla, R. Cesaroni, D. Galli, L. Moscadelli, A. Ahmadi, H. Beuther, S. Etoka, C. Goddi, P. D. Klaassen, R. Kuiper, M. S. N. Kumar, A. Lorenzani, T. Peters, Á. Sánchez-Monge, P. Schilke, F. van der Tak, S. Vig

Publikováno v: Astronomy and astrophysics, 659:A81. EDP Sciences
Astronomy & Astrophysics, 659:A81

Context. To better understand the formation of high-mass stars, it is fundamental to investigate how matter accretes onto young massive stars, how it is ejected, and how all this differs from the low-mass case. The massive protocluster G31.41+0.31 is

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6d18604d4cc26d2b676b37d9a5c67be2
https://research.rug.nl/en/publications/4da4b8a1-a30f-458f-af11-4fa9cc4baf57

ATOMIUM: ALMA tracing the origins of molecules in dust forming oxygen rich M-type stars: Motivation, sample, calibration, and initial results

Autor: C. A. Gottlieb, L. Decin, A. M. S. Richards, F. De Ceuster, W. Homan, S. H. J. Wallström, T. Danilovich, T. J. Millar, M. Montargès, K. T. Wong, I. McDonald, A. Baudry, J. Bolte, E. Cannon, E. De Beck, A. de Koter, I. El Mellah, S. Etoka, D. Gobrecht, M. Gray, F. Herpin, M. Jeste, P. Kervella, T. Khouri, E. Lagadec, S. Maes, J. Malfait, K. M. Menten, H. S. P. Müller, B. Pimpanuwat, J. M. C. Plane, R. Sahai, M. Van de Sande, L. B. F. M. Waters, J. Yates, A. Zijlstra

Publikováno v: Gottlieb, C A, Decin, L, Richards, A M S, De Ceuster, F, Homan, W, Wallström, S H J, Danilovich, T, Millar, T J, Montargès, M, Wong, K T, Mcdonald, I, Baudry, A, Bolte, J, Cannon, E, De Beck, E, De Koter, A, El Mellah, I, Etoka, S, Gobrecht, D, Gray, M, Herpin, F, Jeste, M, Kervella, P, Khouri, T, Lagadec, E, Maes, S, Malfait, J, Menten, K M, Müller, H S P, Pimpanuwat, B, Plane, J M C, Sahai, R, Van De Sande, M, Waters, L B F M, Yates, J & Zijlstra, A 2022, ' ATOMIUM: ALMA tracing the origins of molecules in dust forming oxygen rich M-type stars : Motivation, sample, calibration, and initial results ', Astronomy & Astrophysics, vol. 660, pp. A94 . https://doi.org/10.1051/0004-6361/202140431
Astronomy & Astrophysics

This overview paper presentsATOMIUM, a Large Programme in Cycle 6 with the Atacama Large Millimeter/submillimeter Array (ALMA). The goal ofATOMIUMis to understand the dynamics and the gas phase and dust formation chemistry in the winds of evolved asy

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dc5939de8890ed289bf09c50947ab1a5
http://arxiv.org/abs/2112.04399

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