Results 91 to 100 of about 180 (127)
A <i>λ</i> 3 mm and 1 mm line survey toward the yellow hypergiant IRC +10420: N-rich chemistry and IR flux variations. [PDF]
Astron Astrophys, 2016 Quintana-Lacaci G +6 more
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Search for Chirality in Hydrogenated Magnesium Nanosilicates: A DFT and TD-DFT Investigation. [PDF]
J Phys Chem AStelmach KB, Dukes CA, Garrod RT.
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Core-collapse supernovae as cosmic ray sources. [PDF]
Mon Not R Astron Soc, 2018 Marcowith A +4 more
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The Evolution of Compact Binary Star Systems. [PDF]
Living Rev Relativ, 2014 Postnov KA, Yungelson LR.
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Young Stellar Objects in the Massive Star-forming Regions W51 and W43. [PDF]
Astrophys J, 2017 Saral G +8 more
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X-ray emission from SN 2012ca: A Type Ia-CSM supernova explosion in a dense surrounding medium. [PDF]
Mon Not R Astron Soc, 2018 Bochenek CD +6 more
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Gamma-ray bursts and their use as cosmic probes. [PDF]
R Soc Open Sci, 2017 Schady P.
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Annual Review of Astronomy and Astrophysics, 1987
This paper reviews the current status of knowledge regarding the basic physical and chemical properties of Wolf—Rayet stars; their overall mass loss and stellar wind characteristics and current ideas about their evolutionary status. WR stars are believed to be the evolved descendents of massive O—type stars, in which extensive mass loss reveals ...
Allan J. Willis, Catharine D. Garmany
+4 more sources
This paper reviews the current status of knowledge regarding the basic physical and chemical properties of Wolf—Rayet stars; their overall mass loss and stellar wind characteristics and current ideas about their evolutionary status. WR stars are believed to be the evolved descendents of massive O—type stars, in which extensive mass loss reveals ...
Allan J. Willis, Catharine D. Garmany
+4 more sources
Annual Review of Astronomy and Astrophysics, 1966
Wolf-Rayet stars are few in number and their spectra are easily recognised, for wide emission lines dominate the spectrum. The Wolf-Rayet stars form one of the few groups of stars which are named after astronomers. Wolf and Rayet (1867) at the Paris Observatory used a visual spectrometer to examine the spectra of stars and they noted that the spectra ...
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Wolf-Rayet stars are few in number and their spectra are easily recognised, for wide emission lines dominate the spectrum. The Wolf-Rayet stars form one of the few groups of stars which are named after astronomers. Wolf and Rayet (1867) at the Paris Observatory used a visual spectrometer to examine the spectra of stars and they noted that the spectra ...
openaire +1 more source