Zobrazeno 1 - 10
of 26
pro vyhledávání: '"Sophie Van Eck"'
Publikováno v:
Universe, Vol 8, Iss 4, p 220 (2022)
The foundations of stellar nucleosynthesis have been established more than 70 years ago. Since then, much progress has been made, both on the theoretical side, with stellar evolution and nucleosynthesis models of increasing complexity, using more and
Externí odkaz:
https://doaj.org/article/74f40c9c6f4e4fa7a8229f488dce0a89
Autor:
Thibault Merle, Adrian S. Hamers, Sophie Van Eck, Alain Jorissen, Mathieu Van der Swaelmen, Karen Pollard, Rodolfo Smiljanic, Dimitri Pourbaix, Tomaž Zwitter, Gregor Traven, Gerry Gilmore, Sofia Randich, Anaïs Gonneau, Anna Hourihane, Germano Sacco, C. Clare Worley
Publikováno v:
Nature Astronomy. 6:681-688
Binaries have received much attention as possible progenitors of Type Ia supernova (SNIa) explosions, but long-term gravitational effects in tight triple or quadruple systems could also play a key role in producing SNIa. Here we report on the propert
Autor:
Ana Escorza, Drisya Karinkuzhi, Alain Jorissen, Sophie Van Eck, Joan Schmelz, Gerrit Verschuur, Henri Boffin, Robert De Rosa, Hans Van Winckel
Neutron stars are possible end products of massive star evolution (M ≥ 8 Msun). They are exotic astronomical objects observed with masses between 1.2 and 2.35 Msun and typically emitting at radio and X-ray wavelengths, especially when being young a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4466a8e7062fcd4b9afc63d7183f253f
https://doi.org/10.21203/rs.3.rs-1979121/v1
https://doi.org/10.21203/rs.3.rs-1979121/v1
Autor:
Maria Sofia Randich, Gerard Gilmore, Anna Houriane, Thibault Merle, Mathieu Van der Swaelmen, Dimitri Pourbaix, Adrian Hamers, Alain Jorissen, Karen Pollard, Sophie Van Eck, Gregor Traven, C. C. Worley, G. G. Sacco, Tomaz Zwitter, Anais Gonneau, Rodolfo Smiljanic
Stars often form in multiple systems and may follow a complex evolution involving mass transfer and collisions, leading to mergers that are possible progenitors of Type Ia supernovae (SNe) [1, 2]. The progenitors of such explosions are still highly d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::65b0c28983da145c79d2ada51502fe60
https://doi.org/10.21203/rs.3.rs-1050702/v1
https://doi.org/10.21203/rs.3.rs-1050702/v1
Autor:
Sophie Van Eck, Hans Van Winckel, Lionel Siess, George Wallerstein, Bertrand Plez, Michel Godefroid, Alain Jorissen, S. Shetye, Stéphane Goriely
Publikováno v:
Astronomy & astrophysics, 650
S stars are late-type giants that are transition objects between M-type stars and carbon stars on the asymptotic giant branch (AGB). They are classified into two types: intrinsic or extrinsic, based on the presence or absence of technetium (Tc). The
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9c2272fda41aaa7e56dc8ffddbff945c
http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/322799
http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/322799
Autor:
Thomas Masseron, Lionel Siess, D. Karinkuzhi, Stéphane Goriely, Thibault Merle, Sophie Van Eck, Alain Jorissen
Publikováno v:
Journal of astrophysics and astronomy
Journal of astrophysics and astronomy, 41 (1
Journal of astrophysics and astronomy, 41 (1
We present an on-going project consisting of analysis of a sample of twenty-five metal-poor stars, most of them carbon-enriched and thus tagged carbon-enhanced metal-poor (CEMP) stars, observed with the high-resolution HERMES spectrograph mounted on
Autor:
Claudia Travaglio, Andreea S. Font, Maria Lugaro, Selma E. de Mink, Jacqueline den Hartogh, Artemis Spyrou, P. Gina Isar, Ewa Niemczura, Remo Collet, Birgitta Nordström, Panagiota Papakonstantinou, Marialuisa Aliotta, Sanjana Curtis, W. Chantereau, Mariya Yavahchova, Friedrich-Karl Thielemann, Christine V. Hampton, Thomas Rauscher, A. Ćiprijanović, Claudia Lederer-Woods, Nalan Özkan, Etienne A. Kaiser, Anu Kankainen, Chiaki Kobayashi, Marcella Di Criscienzo, Aparna Venkatesan, Sophie Van Eck
Publikováno v:
Springer proceedings in physics, 219
Springer Proceedings in Physics ISBN: 9783030138752
Springer Proceedings in Physics ISBN: 9783030138752
Female role models reduce the impact on women of stereotype threat, i.e. of being at risk of conforming to a negative stereotype about one’s social, gender, or racial group (Fine in Delusion of Gender. W.W. Norton & Co. NY, p. 36, 2010 [1]; St
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1890dcfa772122cec903470b61063cbb
http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/296706
http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/296706
Publikováno v:
Proceedings of the International Astronomical Union. 12:345-347
S-type stars are late-type giants enhanced with s-process elements originating either from nucleosynthesis during the Asymptotic Giant Branch (AGB) or from a pollution by a binary companion. The former are called intrinsic S stars, and the latter ext
Autor:
Markus Wittkowski, Sophie Van Eck, Richard I. Anderson, Alain Jorissen, Andrea Chiavassa, B. Freytag, K. Kravchenko, Ulli Käufl
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, ⟨10.1051/0004-6361/202038581⟩
Astronomy & astrophysics, 642
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, ⟨10.1051/0004-6361/202038581⟩
Astronomy & astrophysics, 642
Context. Asymptotic giant branch (AGB) stars are characterized by substantial mass loss, however the mechanism behind it not yet fully understood. The knowledge of the structure and dynamics of AGB-star atmospheres is crucial to better understanding
Publikováno v:
Astrometry and Astrophysics in the Gaia sky. Cambridge University Press
The Gaia-ESO survey (GES; Gilmore et al. (2012), Randich et al. (2013)) is a spectroscopic survey complementing the Gaia mission to bring accurate radial velocities and chemical abundances for 105 stars. Merle et al. (submitted to A&A; see also this
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2cede3e90901993548999a56df5ea489
http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/280597
http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/280597