Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Silke Maes"'
Publikováno v:
The Astrophysical Journal, Vol 969, Iss 2, p 79 (2024)
The chemistry of an astrophysical environment is closely coupled to its dynamics, the latter often found to be complex. Hence, to properly model these environments a 3D context is necessary. However, solving chemical kinetics within a 3D hydro simula
Externí odkaz:
https://doaj.org/article/a8732da99e6a4513ae50cf23d5b5a98a
Autor:
Taissa Danilovich, Jolien Malfait, Marie Van de Sande, Miguel Montargès, Pierre Kervella, Frederik De Ceuster, Arnout Coenegrachts, Tom Millar, Anita Richards, Leen Decin, Carl Gottlieb, Christophe Pinte, Elvire De Beck, Daniel Price, Jan Bolte, Karl Menten, Alain Baudry, Alexander de Koter, Sandra Etoka, David Gobrecht, Malcolm Gray, Fabrice Herpin, Manali Jeste, Eric Lagadec, Silke Maes, Iain McDonald, Louise Marinho, Holger Müller, Bannawit Pimpanuwat, John Plane, Raghvendra Sahai, Sofia Wallström, Ka Tat Wong, Jeremy Yates, Albert Zijlstra
Binary interactions have been proposed to explain a variety of circumstellar structures seen around evolved stars, including asymptotic giant branch (AGB) stars and planetary nebulae. Studies resolving the circumstellar envelopes of AGB stars have re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8c8fd52ec108fa97e3b8712274100687
https://doi.org/10.21203/rs.3.rs-2749842/v1
https://doi.org/10.21203/rs.3.rs-2749842/v1
Autor:
Jolien Malfait, Silke Maes, Ward Homan, Jan Bolte, Lionel Siess, Frederik De Ceuster, Leen Decin
With the use of high-resolution ALMA observations, complex structures that resemble those observed in post-AGB stars and planetary nebulae are detected in the circumstellar envelopes of low-mass evolved stars. These deviations from spherical symmetry
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::888568c5d6aa9aeeab147b7c889a4c70
http://arxiv.org/abs/2207.14032
http://arxiv.org/abs/2207.14032
Autor:
Silke Maes, Lionel Siess, Ward Homan, Jolien Malfait, Frederik De Ceuster, Thomas Ceulemans, Dion Donné, Mats Esseldeurs, Leen Decin
Publikováno v:
Proceedings of the International Astronomical Union. 16:227-233
Low- and intermediate mass stars experience a significant mass loss during the last phases of their evolution, which obscures them in a vast, dusty envelope. Although it has long been thought this envelope is generally spherically symmetric in shape,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2c1d9be1162365260dd98e7dbe89da11
https://doi.org/10.1017/s1743921322000217
https://doi.org/10.1017/s1743921322000217