Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Wang Tianding"'
Mass loss is a crucial process that affects the observational properties, evolution path and fate of highly evolved stars. However, the mechanism of mass loss is still unclear, and the mass-loss rate (MLR) of red supergiant stars (RSGs) requires furt
Externí odkaz:
http://arxiv.org/abs/2401.03778
Autor:
Yang, Ming, Bonanos, Alceste Z., Jiang, Biwei, Zapartas, Emmanouil, Gao, Jian, Ren, Yi, Lam, Man I, Wang, Tianding, Maravelias, Grigoris, Gavras, Panagiotis, Wang, Shu, Chen, Xiaodian, Tramper, Frank, de Wit, Stephan, Chen, Bingqiu, Wen, Jing, Liu, Jiaming, Tian, Hao, Antoniadis, Konstantinos, Luo, Changqing
Publikováno v:
A&A 676, A84 (2023)
We assemble the most complete and clean red supergiant (RSG) sample (2,121 targets) so far in the Small Magellanic Cloud (SMC) with 53 different bands of data to study the MLR of RSGs. In order to match the observed spectral energy distributions (SED
Externí odkaz:
http://arxiv.org/abs/2304.01835
The infrared excess from OB stars are commonly considered as contributions from ionized stellar wind or circumstellar dust. With the newly published LAMOST-OB catalog and GOSSS data, this work steps further on understanding the infrared excess of OB
Externí odkaz:
http://arxiv.org/abs/2207.06961
This work establishes the most complete sample of red supergiants (RSGs) in twelve low-mass galaxies (WLM, IC 10, NGC 147, NGC 185, IC 1613, Leo A, Sextans B, Sextans A, NGC 6822, Pegasus Dwarf, SMC and LMC) of the Local Group, which forms the solid
Externí odkaz:
http://arxiv.org/abs/2110.08793
Publikováno v:
MATEC Web of Conferences, Vol 34, p 02012 (2015)
This paper presents a new generation algorithm for tool path based on the optimization of traditional algorithms. Then, the tool path on an impeller is generated with UG software, and it is used to make contrasts and verifications for the effect of o
Externí odkaz:
https://doaj.org/article/4aadaa1ab21341cd8a70448bdfff9e6a
Mass loss is an important activity for red supergiants (RSGs) which can influence their evolution and final fate. Previous estimations of mass loss rates (MLRs) of RSGs exhibit significant dispersion due to the difference in method and the incomplete
Externí odkaz:
http://arxiv.org/abs/2103.05263
The aim of this paper is to establish a complete sample of red supergiants (RSGs) in M31 and M33. The member stars of the two galaxies are selected from the near-infrared (NIR) point sources after removing the foreground dwarfs from their obvious bra
Externí odkaz:
http://arxiv.org/abs/2011.12051
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