Zobrazeno 1 - 10
of 14
pro vyhledávání: '"Erin R Higgins"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 516:4052-4065
The most massive stars dominate the chemical enrichment, mechanical and radiative feedback, and energy budget of their host environments. Yet how massive stars initially form and how they evolve throughout their lives is ambiguous. The mass loss of t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::91c1d56e2f445005c80e3ae59b32267a
https://doi.org/10.1093/mnras/stac2485
https://doi.org/10.1093/mnras/stac2485
Very massive stars (VMS) dominate the physics of young clusters due to their ionising radiation and extreme stellar winds. It is these winds that determine their lifepaths until expiration. Observations in the Arches cluster show that VMS all have si
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::77410d75134d8bdae18a3a870317d940
http://arxiv.org/abs/2205.09125
http://arxiv.org/abs/2205.09125
Autor:
Andreas A. C. Sander, Jorick S. Vink, Erin R. Higgins, Tomer Shenar, Wolf-Rainer Hamann, Helge Todt
Classical Wolf-Rayet (WR) stars mark an important stage in the late evolution of massive stars. As hydrogen-poor massive stars, these objects have lost their outer layers, while still losing further mass through strong winds indicated by their promin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dcae7d3e8916bf683a3d95574637256b
http://arxiv.org/abs/2202.04671
http://arxiv.org/abs/2202.04671
Autor:
Sam Geen, Poojan Agrawal, Paul A. Crowther, B. W. Keller, Alex de Koter, Zsolt Keszthelyi, Freeke van de Voort, Ahmad A. Ali, Frank Backs, Lars Bonne, Vittoria Brugaletta, Annelotte Derkink, Sylvia Ekström, Yvonne A. Fichtner, Luca Grassitelli, Ylva Götberg, Erin R. Higgins, Eva Laplace, Kong You Liow, Marta Lorenzo, Anna F. McLeod, Georges Meynet, Megan Newsome, G. André Oliva, Varsha Ramachandran, Martin P. Rey, Steven Rieder, Emilio Romano-Díaz, Gautham Sabhahit, Andreas A. C. Sander, Rafia Sarwar, Hanno Stinshoff, Mitchel Stoop, Dorottya Szécsi, Maxime Trebitsch, Jorick S. Vink, Ethan Winch
Publikováno v:
Publications of the Astronomical Society of the Pacific, 2023, Vol.135(1044) [Peer Reviewed Journal]
Stars strongly impact their environment, and shape structures on all scales throughout the universe, in a process known as “feedback.” Due to the complexity of both stellar evolution and the physics of larger astrophysical structures, there remai
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::af74de90d16ee3341e1f94bbe9b23a33
https://doi.org/10.1088/1538-3873/acb6b5
https://doi.org/10.1088/1538-3873/acb6b5
The Humphreys-Davidson (HD) limit sets the boundary between evolutionary channels of massive stars that either end their lives as red supergiants (RSGs) or as the hotter blue supergiants (BSGs) and Wolf-Rayet stars. Mixing in the envelopes of massive
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e8e51d1618c936f96d98df69e54d3426
At the end of its life, a very massive star is expected to collapse into a black hole. The recent detection of an 85 Msun black hole from the gravitational wave event GW 190521 appears to present a fundamental problem as to how such heavy black holes
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4fde89d00bd937b7a936d343ec8c849e
http://arxiv.org/abs/2010.11730
http://arxiv.org/abs/2010.11730
At the end of its life, a very massive star is expected to collapse into a black hole. The masses of these black holes are pivotal for our understanding of the evolution and fate of these stars, as well as for galaxy evolution and the build-up of bla
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::665a0756c3c46707c8e441cd8d0ca79a
https://doi.org/10.21203/rs.3.rs-80351/v1
https://doi.org/10.21203/rs.3.rs-80351/v1
Autor:
Erin R. Higgins, Jorick S. Vink
Current massive star evolution grids are not able to simultaneously reproduce the empirical upper luminosity limit of red supergiants, the Humphrey-Davidson (HD) limit at high and low metallicity. In this study, we provide a better understanding of w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::79cc916f551e1729f617fb44214d1b5a
http://arxiv.org/abs/2002.07204
http://arxiv.org/abs/2002.07204
Autor:
Jorick S. Vink, Erin R. Higgins
Publikováno v:
Proceedings of the International Astronomical Union. 14:480-485
Massive star evolution is dominated by key physical processes such as mass loss, convection and rotation, yet these effects are poorly constrained, even on the main sequence. We utilise a detached, eclipsing binary HD166734 as a testbed for single st
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5cd0234377feb97239d9ab7d41eb2fd9
https://doi.org/10.1017/s1743921319001170
https://doi.org/10.1017/s1743921319001170
Autor:
Jorick S. Vink, Erin R. Higgins
Publikováno v:
Astronomy & Astrophysics. 622:A50
We aim to constrain massive star evolution models using the unique testbed eclipsing binary HD166734 with new grids of MESA stellar evolution models, adopting calibrated prescriptions of overshooting, mass loss, and rotation. We introduce a novel too
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a7fbbe4ae27108f8780f3c6fa697fba9
https://doi.org/10.1051/0004-6361/201834123
https://doi.org/10.1051/0004-6361/201834123