Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Andreas A. C. Sander"'
Autor:
Ilyse Clark, Danielle A. Berg, Claus Leitherer, Karla Z. Arellano-Córdova, Andreas A. C. Sander
Publikováno v:
The Astrophysical Journal, Vol 964, Iss 1, p 25 (2024)
We present an analysis of the effects of spectral resolution and aperture scale on derived galaxy properties using far-ultraviolet (FUV) spectra of local star-forming galaxies from the International Ultraviolet Explorer ( R ∼ 250, field of view (FO
Externí odkaz:
https://doaj.org/article/2d0ec0f9b1df4ecfaeb991d562ff659e
Autor:
Ryan M. Lau, Jason Wang, Matthew J. Hankins, Thayne Currie, Vincent Deo, Izumi Endo, Olivier Guyon, Yinuo Han, Anthony P. Jones, Nemanja Jovanovic, Julien Lozi, Anthony F. J. Moffat, Takashi Onaka, Garreth Ruane, Andreas A. C. Sander, Samaporn Tinyanont, Peter G. Tuthill, Gerd Weigelt, Peredur M. Williams, Sebastien Vievard
Publikováno v:
The Astrophysical Journal, Vol 951, Iss 2, p 89 (2023)
Wolf-Rayet (WR) 140 is the archetypal periodic dust-forming colliding-wind binary that hosts a carbon-rich WR (WC) star and an O-star companion with an orbital period of 7.93 yr and an orbital eccentricity of 0.9. Throughout the past few decades, mul
Externí odkaz:
https://doaj.org/article/9bd216773ffa43d7a08a9226c15c504b
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
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:
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
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