Zobrazeno 1 - 10
of 130
pro vyhledávání: '"Geraldine J. Peters"'
Publikováno v:
The Astronomical Journal, Vol 165, Iss 5, p 203 (2023)
Close binary interactions may play a critical role in the formation of the rapidly rotating Be stars. Mass transfer can result in a mass gainer star spun up by the accretion of mass and angular momentum, while the mass donor is stripped of its envelo
Externí odkaz:
https://doaj.org/article/3acd7db633654a9dba2dd6288bf32488
Autor:
Geraldine J. Peters, Kenneth G. Gayley, Richard Ignace, Carol E. Jones, Yaël Nazé, Nicole St-Louis, Heloise Stevance, Jorick S. Vink, Noel D. Richardson, Jennifer L. Hoffman, Jamie R. Lomax, Tomer Shenar, Andrew G. Fullard, Paul A. Scowen
Publikováno v:
Astrophysics and Space Science, 367(12):119. Springer Netherlands
One objective of the Polstar spectropolarimetry mission is to characterize the degree of nonconservative mass transfer that occurs at various stages of binary evolution, from the initial mass reversal to the late Algol phase. The proposed instrument
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::268847bc36c3758f5984ff13ca08d021
https://dare.uva.nl/personal/pure/en/publications/ultraviolet-spectropolarimetry(f558863d-b43f-4c3f-849d-f5f6bc7c8afd).html
https://dare.uva.nl/personal/pure/en/publications/ultraviolet-spectropolarimetry(f558863d-b43f-4c3f-849d-f5f6bc7c8afd).html
Publikováno v:
Proceedings of the International Astronomical Union. 14:143-145
A recent survey of the far-ultraviolet spectra of 264 B-emission line stars has revealed 16 systems with hot companions that are the stripped down remains of a former mass donor star. Some of these will probably become Be + neutron star X-ray binarie
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2f2dd6ad56efe0589ec2bb922632aaa7
https://doi.org/10.1017/s1743921319002217
https://doi.org/10.1017/s1743921319002217
Autor:
Y. Götberg, Steve B. Howell, Douglas R. Gies, Kathryn V. Lester, S. Drew Chojnowski, Geraldine J. Peters, Luqian Wang
Publikováno v:
The Astronomical Journal. 161:248
The B-emission line stars are rapid rotators that were probably spun up by mass and angular momentum accretion through mass transfer in an interacting binary. Mass transfer will strip the donor star of its envelope to create a small and hot subdwarf
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7ba649ca2eddadfd43fbd7e063b8cec9
https://doi.org/10.3847/1538-3881/abf144
https://doi.org/10.3847/1538-3881/abf144
Autor:
Ronald E. Mennickent, Juan Fabregat, M. Virginia McSwain, Richard H. D. Townsend, Carol E. Jones, Karen S. Bjorkman, Coralie Neiner, Geraldine J. Peters, Philippe Stee
Publikováno v:
Proceedings of the International Astronomical Union
Proceedings of the International Astronomical Union, 2011, 7 (T28A), pp.199-202. ⟨10.1017/S1743921312002803⟩
Proceedings of the International Astronomical Union, 2011, 7 (T28A), pp.199-202. ⟨10.1017/S1743921312002803⟩
The meeting of the Working Group on Active B Stars consisted of a business session followed by a scientific session containing nine talks. The titles of the talks and their presenters are listed below. We plan to publish a series of articles containi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f7940d5c3edff499cd0170d48115347e
https://doi.org/10.1017/s1743921312002803
https://doi.org/10.1017/s1743921312002803
Autor:
Geraldine J. Peters
Publikováno v:
Proceedings of the International Astronomical Union. 7:47-52
The rapidly-accumulating archives of ground-based and spacecraft data worldwide that are being linked together through the International Virtual Observatory Alliance (IVOA) provide the binary star community with unparalleled opportunities for researc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::92c72c29abf9a5033c9887a9ac9faabf
https://doi.org/10.1017/s1743921311026846
https://doi.org/10.1017/s1743921311026846
Autor:
Geraldine J. Peters, Georges Meynet
Publikováno v:
Proceedings of the International Astronomical Union. 6:79-82
The general discussion following Session 1: Rapid Rotation and Mixing in Active OB Stars is summarized. Topics that focus on observational and theoretical issues are included.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8d320595911dc410786aae015bfa297b
https://doi.org/10.1017/s1743921311010003
https://doi.org/10.1017/s1743921311010003
Autor:
Geraldine J. Peters, Carol E. Jones, Richard D. Townsend, Juan Fabregat, Karen S. Bjorkman, M. Virginia McSwain, Ronald E. Mennickent, Coralie Neiner, Philippe Stee
Publikováno v:
Proceedings of the International Astronomical Union. 6:201-204
The meeting of the Working Group on Active B Stars consisted of a business session followed by a scientific session containing nine talks. The titles of the talks and their presenters are listed below. We plan to publish a series of articles containi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::903e65807b53b53a80a340c6fb9a352d
https://doi.org/10.1017/s1743921310005089
https://doi.org/10.1017/s1743921310005089
Publikováno v:
The Astrophysical Journal. 853:156
There is growing evidence that some Be stars were spun up through mass transfer in a close binary system, leaving the former mass donor star as a hot, stripped-down object. There are five known cases of Be stars with hot subdwarf (sdO) companions tha
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8c68033fd10f30d7b03eb8a57045f5f1
https://doi.org/10.3847/1538-4357/aaa4b8
https://doi.org/10.3847/1538-4357/aaa4b8
Autor:
Geraldine J. Peters
Publikováno v:
Proceedings of the International Astronomical Union. 2:148-153
Contemporary information on the nature of the circumstellar environment in early-type interacting binaries derived from observation is discussed. Emphasis is placed on results from FUV spectroscopy. New spectra from the FUSE spacecraft and earlier FU
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::61a06b1d27d86e80138f6ac988df300b
https://doi.org/10.1017/s174392130700395x
https://doi.org/10.1017/s174392130700395x