Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Rate, G A"'
We provide line luminosities and spectroscopic templates of prominent optical emission lines of 133 Galactic Wolf-Rayet stars by exploiting Gaia DR3 parallaxes and optical spectrophotometry, and provide comparisons with 112 counterparts in the Magell
Externí odkaz:
http://arxiv.org/abs/2301.11297
Autor:
Chené, A. -N., St-Louis, N., Moffat, A. F. J., Schnurr, O., Crowther, P. A., Wade, G. A., Richardson, N. D., Baranec, C., Ziegler, C. A., Law, N. M., Riddle, R., Rate, G. A., Artigau, É., Alecian, E., collaboration, BinaMIcS
Publikováno v:
MNRAS, 484, 5834 (2019)
The hot WN star WR2 (HD6327) has been claimed to have many singular characteristics. To explain its unusually rounded and relatively weak emission line profiles, it has been proposed that WR2 is rotating close to break-up with a magnetically confined
Externí odkaz:
http://arxiv.org/abs/1905.05815
Oxygen sequence Wolf-Rayet stars (WO) are thought to be the final evolution phase of some high mass stars, as such they may be the progenitors of type Ic SNe as well as potential progenitors of broad-lined Ic and long gamma-ray bursts. We present the
Externí odkaz:
http://arxiv.org/abs/1807.02117
Publikováno v:
Monthly Notices of the Royal Astronomical Society; May2023, Vol. 521 Issue 1, p585-612, 28p
Autor:
Rate, G., Crowther, P.A.
We obtain distances to 383 Galactic Wolf-Rayet (WR) stars from Gaia DR2 parallaxes and Bayesian methods, with a prior based on HII regions and dust extinction. Distances agree with those from Bailer-Jones et al. for stars up to 2 kpc from the Sun, th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::6bede9bc58f4046a0f13b281375f7e51
https://eprints.whiterose.ac.uk/156335/1/stz3614.pdf
https://eprints.whiterose.ac.uk/156335/1/stz3614.pdf
Autor:
Chené, A-N, St-Louis, N, Moffat, A F J, Schnurr, O, Crowther, P A, Wade, G A, Richardson, N D, Baranec, C, Ziegler, C A, Law, N M, Riddle, R, Rate, G A, Artigau, É, Alecian, E
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Apr2019, Vol. 484 Issue 4, p5834-5844, 11p
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Oct2018, Vol. 479 Issue 4, p4535-4543, 9p
Vaejovis ocotensis, new species (Figs 1 ���14, 16, 18) Type data. Holotype female (CNAN T-0404) from Cueva del Metate [16 �� 53 ��� 8 ��� N ��� 93 �� 25 ��� 13 ��� W, elevation 900 m], 3.6 km NW Ocuilapa de
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7cc2103129fbbe460374080dac3fcb4e
Publikováno v:
ETSU Faculty Works.
Oxygen sequence Wolf-Rayet stars (WO) are thought to be the final evolution phase of some high-mass stars, as such they may be the progenitors of Type Ic SNe as well as potential progenitors of broad-lined Ic and long gamma-ray bursts. We present the