Zobrazeno 1 - 10
of 16
pro vyhledávání: '"Amber N. Marsh"'
We present a study of the B and Be star populations of the Double Cluster h and chi Persei. Blue optical spectroscopy is used to first measure projected rotational velocity, V sin i, effective surface temperature, T_eff, and surface gravity, log g, f
Externí odkaz:
http://arxiv.org/abs/1209.5771
The recently discovered gamma-ray binary 1FGL J1018.6-5856 has a proposed optical/near-infrared (OIR) counterpart 2MASS 10185560-5856459. We present Stromgren photometry of this star to investigate its photometric variability and measure the reddenin
Externí odkaz:
http://arxiv.org/abs/1109.3692
Autor:
Audrey Wall, M. Virginia McSwain, Steven Waskie, Amber N. Marsh Boyer, Richard J. Hanes, Jonathan Labadie-Bartz
The field of asteroseismology has enjoyed a large swath of data coming from recent missions (e.g., CoRoT, Kepler, K2). This wealth of new data has allowed the field to expand beyond the previous limitation of a few extremely bright and evolved stars.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9a2b9204c4adf2da8ce855ceec84d6ff
Autor:
Tabetha S. Boyajian, Douglas R. Gies, Amber N. Marsh, Mallory S. E. Roberts, Rachael M. Roettenbacher, Erika D. Grundstrom, Michaël De Becker, Christina Aragona, M. Virginia McSwain
Publikováno v:
The Astronomical Journal. 139:857-864
HD 15137 is an intriguing runaway O-type binary system that offers a rare opportunity to explore the mechanism by which it was ejected from the open cluster of its birth. Here we present recent blue optical spectra of HD 15137 and derive a new orbita
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f4ae947d86d976c1a701bec28b7a0421
https://doi.org/10.1088/0004-6256/139/3/857
https://doi.org/10.1088/0004-6256/139/3/857
Publikováno v:
Proceedings of the International Astronomical Union. 5:462-465
We present blue optical spectra of 92 members of h and chi Per obtained with the WIYN telescope at Kitt Peak National Observatory. From these spectra, several stellar parameters were measured for the B-type stars, including V sin i, T_eff, log g_pola
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::711330a9cc684926be6da5a60785db7c
https://doi.org/10.1017/s1743921309991700
https://doi.org/10.1017/s1743921309991700
Autor:
Sherry A. Downie, Priti L. Mishall, Rachel E. Weinstock, Diana Perez, Amber N. Marsh, Xavier H. Quezada, Maximilian C. Stahl
Publikováno v:
Folia Morphologica.
Muscle and tendon variations in the forearm, wrist and hand are commonly reported in the anatomical and surgical literature. They are frequently the source of inflammatory conditions such as de Quervain's tenosynovitis or carpal tunnel syndrome. Duri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::59d011c9f960b115666f9fae3f392a55
https://doi.org/10.5603/fm.a2019.0067
https://doi.org/10.5603/fm.a2019.0067
We present a study of the B and Be star populations of the Double Cluster h and chi Persei. Blue optical spectroscopy is used to first measure projected rotational velocity, V sin i, effective surface temperature, T_eff, and surface gravity, log g, f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::340e5446dd0b6f6aa1eeb20f88c72f24
http://arxiv.org/abs/1209.5771
http://arxiv.org/abs/1209.5771
Autor:
M. Virginia McSwain, Amber N. Marsh, Katelyn M. Hessler, Paul S. Ray, Erika D. Grundstrom, Rachael M. Roettenbacher, Christina Aragona, Tabetha S. Boyajian
LS I +61 303 and LS 5039 are two of only a handful of known high mass X-ray binaries (HMXBs) that exhibit very high energy emission in the MeV-TeV range, and these "gamma-ray binaries" are of renewed interest due to the recent launch of the Fermi Gam
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0795c5dea45457eed0832d4ef0ed7143
http://arxiv.org/abs/0902.4015
http://arxiv.org/abs/0902.4015
Autor:
M. Virginia McSwain, Christina Aragona, Erika D. Grundstrom, Douglas R. Gies, D. W. Wingert, Tabetha S. Boyajian, Stephen J. Williams, Rachael M. Roettenbacher, Amber N. Marsh, E. Victor Garcia
Publikováno v:
Proceedings of the International Astronomical Union. 6:290-291
Massive O- and B-type stars are “cosmic engines” in the Universe and can be the dominant source of luminosity in a galaxy. The class of Be stars are rapidly rotating B-type stars that lose mass in an equatorial, circumstellar disk (Porter & Rivin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ecb550d1af0a4f20c7b8933f64228e59
https://doi.org/10.1017/s1743921311010611
https://doi.org/10.1017/s1743921311010611
Publikováno v:
Astronomical Journal; Dec2012, Vol. 144 Issue 6, p1-10, 10p