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pro vyhledávání: '"A. Rate"'
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
Galactic Wolf-Rayet (WR) star membership of star forming regions can be used to constrain the formation environments of massive stars. Here, we utilise $\textit{Gaia}$ DR2 parallaxes and proper motions to reconsider WR star membership of clusters and
Externí odkaz:
http://arxiv.org/abs/2005.02533
Autor:
Rate, Gemma, Crowther, Paul A.
We obtain distances to 383 Galactic Wolf-Rayet (WR) stars from $\textit{Gaia}$ DR2 parallaxes and Bayesian methods, with a prior based on H$\mathrm{\scriptsize{II}}$ regions and dust extinction. Distances agree with those from Bailer-Jones et al. for
Externí odkaz:
http://arxiv.org/abs/1912.10125
Autor:
Gould, Heath P., Gosnell, Griffith G., Bano, Joseph M., Rate, William R., IV, Sequeira, Sean B., Marchant, Milford H., Jr.
Publikováno v:
In Arthroscopy, Sports Medicine, and Rehabilitation October 2023 5(5)
Autor:
Thach, Keo Sa Rate, Lee, Ji Yong, Ha, My Trang, Cao, Minh Tuan, Nayga, Rodolfo M., Yang, Jae-E
Publikováno v:
In Heliyon October 2023 9(10)
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
The fifth generation (5G) mobile telecommunication network is expected to support Multi- Access Edge Computing (MEC), which intends to distribute computation tasks and services from the central cloud to the edge clouds. Towards ultra-responsive, ultr
Externí odkaz:
http://arxiv.org/abs/1712.00234
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