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pro vyhledávání: '"W. Chantereau"'
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Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 650, pp.A162. ⟨10.1051/0004-6361/202140800⟩
Astronomy and Astrophysics-A&A, 2021, 650, pp.A162. ⟨10.1051/0004-6361/202140800⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 650, pp.A162. ⟨10.1051/0004-6361/202140800⟩
Astronomy and Astrophysics-A&A, 2021, 650, pp.A162. ⟨10.1051/0004-6361/202140800⟩
Multiple populations in globular clusters are usually explained by the formation of stars out of material with a chemical composition that is polluted to different degrees by the ejecta of short-lived, massive stars of various type. Among other thing
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9209d5eab8b82d59982f0d02fa473b31
https://hal.archives-ouvertes.fr/hal-03260790
https://hal.archives-ouvertes.fr/hal-03260790
Autor:
Emanuele Dalessandro, N. Kacharov, W. Chantereau, S. Martocchia, Sebastian Kamann, Nate Bastian, I. Cabrera-Ziri, Carmela Lardo, Maurizio Salaris, Marina Rejkuba, S. S. Larsen
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 505 (4), pp.5389-5402. ⟨10.1093/mnras/stab1590⟩
Monthly Notices of the Royal Astronomical Society, 505, 5389-5402
Monthly Notices of the Royal Astronomical Society, 505, 4, pp. 5389-5402
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 505 (4), pp.5389-5402. ⟨10.1093/mnras/stab1590⟩
Monthly Notices of the Royal Astronomical Society, 505, 5389-5402
Monthly Notices of the Royal Astronomical Society, 505, 4, pp. 5389-5402
We present ESO/VLT FORS2 low resolution spectroscopy of red giant branch stars in three massive, intermediate age ($\sim 1.7-2.3$ Gyr) star clusters in the Large Magellanic Cloud. We measure CH and CN index bands at 4300A, and 3883A, as well as [C/Fe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a71d6c0dbf581fa749e92a2e11dd407b
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.A52. ⟨10.1051/0004-6361/201937212⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.A52. ⟨10.1051/0004-6361/201937212⟩
We investigate the role of binaries and chromospheric emission on HST photometry of globular clusters' stars. We quantify their respective effects on the position of stars in the chromosome map, especially among the first population. We computed atmo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d1384384bcc49dccdc11b0961b8f05e6
http://arxiv.org/abs/2001.07581
http://arxiv.org/abs/2001.07581
Autor:
Sebastian Kamann, Søren S. Larsen, S. Martocchia, Randa Asa'd, Christopher Usher, W. Chantereau, Nate Bastian, Maurizio Salaris, Carmela Lardo, Michael Hilker, I. Cabrera-Ziri
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 494, 1, pp. 332-337
Monthly Notices of the Royal Astronomical Society, 494, 332-337
Monthly Notices of the Royal Astronomical Society, 494, 332-337
Recent work has shown that the properties of multiple populations within massive stellar clusters (i.e., in the extent of their abundance variations as well as the fraction of stars that show the anomalous chemistry) depend on the mass as well as the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::277196f9ad024e464203a6830767741d
http://hdl.handle.net/11585/789324
http://hdl.handle.net/11585/789324
Stars in globular clusters (GCs) lose a non negligible amount of mass during their post-main sequence evolution. This material is then expected to build up a substantial intra-cluster medium (ICM) within the GC. However, the observed gas content in G
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2d520c428eff9520884fb97c60619190
Autor:
Maurizio Salaris, W. Chantereau, S. Martocchia, Ricardo P. Schiavon, Carmela Lardo, Christopher Usher, Michael Hilker, I. Cabrera-Ziri, Sebastian Kamann, Søren S. Larsen, Randa Asa'd, Nate Bastian
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters, 489, 1, pp. L80-L85
Monthly Notices of the Royal Astronomical Society: Letters, 489, L80-L85
Monthly Notices of the Royal Astronomical Society: Letters, 489, L80-L85
The presence of star-to-star light-element abundance variations (a.k.a. multiple populations, MPs) appears to be ubiquitous within old and massive clusters in the Milky Way and all studied nearby galaxies. Most previous studies have focussed on resol
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::af99125af259ff1e775a51b674f94cd6
http://arxiv.org/abs/1909.01404
http://arxiv.org/abs/1909.01404
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:
Monthly Notices of the Royal Astronomical Society
Intermediate-age star clusters in the Magellanic Clouds harbour signatures of the multiple stellar populations long thought to be restricted to old globular clusters. We compare synthetic horizontal branch models with Hubble Space Telescope photometr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d963e1c534a8ba9b00264ca3470eecb5
http://arxiv.org/abs/1902.01806
http://arxiv.org/abs/1902.01806
Autor:
Carmela Lardo, Imants Platais, Florian Niederhofer, V. Kozhurina-Platais, Emanuele Dalessandro, Christopher Usher, Maurizio Salaris, Michael Hilker, I. Cabrera-Ziri, Doug Geisler, S. Martocchia, Nate Bastian, N. Kacharov, S. S. Larsen, Alessio Mucciarelli, W. Chantereau
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 487, 4, pp. 5324-5334
Monthly Notices of the Royal Astronomical Society, 487, 5324-5334
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 487, 5324-5334
Monthly Notices of the Royal Astronomical Society
In our HST photometric survey, we have been searching for multiple stellar populations (MPs) in Magellanic Clouds (MCs) massive star clusters which span a significant range of ages ($\sim 1.5-11$ Gyr). In the previous papers of the series, we have sh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::66ee6d111a6c8b4f1d5fa5b04eb6bac1
https://hdl.handle.net/2066/205632
https://hdl.handle.net/2066/205632