Zobrazeno 1 - 10
of 80
pro vyhledávání: '"Stephen L. W. McMillan"'
Autor:
Sean C. Lewis, Stephen L. W. McMillan, Mordecai-Mark Mac Low, Claude Cournoyer-Cloutier, Brooke Polak, Martijn J. C. Wilhelm, Aaron Tran, Alison Sills, Simon Portegies Zwart, Ralf S. Klessen, Joshua E. Wall
Publikováno v:
The Astrophysical Journal, Vol 944, Iss 2, p 211 (2023)
Feedback from massive stars plays an important role in the formation of star clusters. Whether a very massive star is born early or late in the cluster formation timeline has profound implications for the star cluster formation and assembly processes
Externí odkaz:
https://doaj.org/article/7fb8d7108d87481eac0b5e5b85242998
Autor:
Claude Cournoyer-Cloutier, Alison Sills, William E Harris, Sabrina M Appel, Sean C Lewis, Brooke Polak, Aaron Tran, Martijn J C Wilhelm, Mordecai-Mark Mac Low, Stephen L W McMillan, Simon Portegies Zwart
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 521:1338-1352
We perform simulations of star cluster formation to investigate the morphological evolution of embedded star clusters in the earliest stages of their evolution. We conduct our simulations with Torch, which uses the Amuse framework to couple state-of-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::72105133e02635e363e8a28ac5bd2e94
https://doi.org/10.1093/mnras/stad568
https://doi.org/10.1093/mnras/stad568
Autor:
Sean C. Lewis, Stephen L. W. McMillan, Mordecai-Mark Mac Low, Claude Cournoyer-Cloutier, Brooke Polak, Martijn J. C. Wilhelm, Aaron Tran, Alison Sills, Simon Portegies Zwart, Ralf S. Klessen, Joshua E. Wall
Feedback from massive stars plays an important role in the formation of star clusters. Whether a very massive star is born early or late in the cluster formation timeline has profound implications for the star cluster formation and assembly processes
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::99a35ff5ecffb29c582dab8d67de34ba
http://arxiv.org/abs/2212.01465
http://arxiv.org/abs/2212.01465
Publikováno v:
Astronomy & Astrophysics, 659:A86
In self-gravitating $N$-body systems, small perturbations introduced at the start, or infinitesimal errors that are produced by the numerical integrator or are due to limited precision in the computer, grow exponentially with time. For Newton's gravi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7e9bf36580653fd983a30ced911c6b07
https://ora.ox.ac.uk/objects/uuid:b0bcfe48-872c-4e81-8fdf-0c1eaed2e24b
https://ora.ox.ac.uk/objects/uuid:b0bcfe48-872c-4e81-8fdf-0c1eaed2e24b
Autor:
Martijn J. C. Wilhelm, Simon Portegies Zwart, Claude Cournoyer-Cloutier, Sean Lewis, Brooke Polak, Aaron Tran, Mordecai-Mark Mac Low, Stephen L. W. McMillan
Publikováno v:
Proceedings of the International Astronomical Union. 16:300-305
Stars form in clusters, while planets form in gaseous disks around young stars. Cluster dissolution occurs on longer time scales than disk dispersal. Planet formation thus typically takes place while the host star is still inside the cluster. We expl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f199bfa1d1c28d67e4ec8b25583dff5e
https://doi.org/10.1017/s1743921322001727
https://doi.org/10.1017/s1743921322001727
Autor:
Mordecai-Mark Mac Low, Ralf S. Klessen, Andrew Pellegrino, Simon Portegies Zwart, Stephen L. W. McMillan, Joshua E. Wall
Publikováno v:
The Astrophysical Journal, 904(2), 192
Understanding the formation of stellar clusters requires following the interplay between gas and newly formed stars accurately. We therefore couple the magnetohydrodynamics code FLASH to the N-body code ph4 and the stellar evolution code SeBa using t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5befe351aedb9fbe9292c7d0c7f5760b
https://hdl.handle.net/1887/3134184
https://hdl.handle.net/1887/3134184
Autor:
William E. Harris, Mordecai-Mark Mac Low, Aaron Tran, Simon Portegies Zwart, Stephen L. W. McMillan, Sean Lewis, Alison Sills, Joshua E. Wall, Claude Cournoyer-Cloutier
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 501(3), 4464-4478
The fraction of stars in binary systems within star clusters is important for their evolution, but what proportion of binaries form by dynamical processes after initial stellar accretion remains unknown. In previous work, we showed that dynamical int
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d3a3f0e0a8e003e89904a527770c37b9
http://arxiv.org/abs/2011.06105
http://arxiv.org/abs/2011.06105
Autor:
Aaron M. Geller, Stephen L. W. McMillan, Jonathan D. Thornton, Joseph P. Glaser, Mark R. Giovinazzi
To fully understand the diverse population of exoplanets, we must study their early lives within open clusters, the birthplace of most stars with masses $>0.5M_\odot$ (including those currently in the field). Indeed, when we observe planets within cl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ca87268a43cf4fffd6e6477a987be7e0
Publikováno v:
Astronomy and Astrophysics (0004-6361), 624, A120
Astronomy and Astrophysics (0004-6361)
Astronomy and Astrophysics (0004-6361)
We perform a simulation using the Astrophysical Multipurpose Software Environment of the Orion Trapezium star cluster in which the evolution of the stars and the dynamics of planetary systems are taken into account. The initial conditions from earlie
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e3e73857daefa37104aaa92b880217df
http://hdl.handle.net/1887/84971
http://hdl.handle.net/1887/84971
Autor:
Mordecai-Mark Mac Low, Joshua E. Wall, Ralf S. Klessen, Stephen L. W. McMillan, Simon Portegies Zwart
Publikováno v:
Astrophysical Journal (0004-637X), 887(1), 62
We describe a star cluster formation model that includes individual star formation from self-gravitating, magnetized gas, coupled to collisional stellar dynamics. The model uses the Astrophysical Multi-purpose Software Environment (AMUSE) to integrat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6e656a70c0efba4db9fbdfac00f06210
http://arxiv.org/abs/1901.01132
http://arxiv.org/abs/1901.01132