创新 发表于 2025-3-26 22:34:29

http://reply.papertrans.cn/31/3029/302865/302865_31.png

deciduous 发表于 2025-3-27 03:25:38

Robert P. Trueblood,John N. Lovett Jr.Contrary to the results of some investigators, the ratio of terminal to escape velocities (V∞/Vesc) observed for the winds in early-type stars is found to be linearly correlated with log г — г being the ratio of stellar to Eddington’s luminosities.

FRAX-tool 发表于 2025-3-27 08:22:57

http://reply.papertrans.cn/31/3029/302865/302865_33.png

执拗 发表于 2025-3-27 10:05:21

Is a Stellar Wind Inherent in WR-Stars Throughout the Whole of their Evolution?In addition to certain manifestation of a stellar wind during steady states of WR-stars that we have heard here about I have two notes on their extremal stages of evolution which may be also connected to such a hydrodynamical event.

colony 发表于 2025-3-27 14:27:25

http://reply.papertrans.cn/31/3029/302865/302865_35.png

令人悲伤 发表于 2025-3-27 21:14:59

Mass Outflow in AG Carinae and a Comparison with P CygniAG Car is a variable supergiant surrounded by a small ring nebula. Its ultraviolet and optical spectrum, and UV to IR energy distribution are similar to those of P Cyg with v. = -290 km s.. Also the strength of the 2200 A band is the same and suggests E(B-V) = 0.55 both stars. The possible variability of the infrared flux is discussed.

Override 发表于 2025-3-28 01:39:33

Mass Loss from Hot Stars Below the Main SequenceThe evolutionary implications of mass loss from post-asymptotic giant branch stars is discussed, with reference to the UV observations of sdO’s.

注视 发表于 2025-3-28 04:38:27

http://reply.papertrans.cn/31/3029/302865/302865_38.png

Mercantile 发表于 2025-3-28 06:40:49

http://reply.papertrans.cn/31/3029/302865/302865_39.png

忧伤 发表于 2025-3-28 13:17:17

http://reply.papertrans.cn/31/3029/302865/302865_40.png
页: 1 2 3 [4] 5 6 7
查看完整版本: Titlebook: Effects of Mass Loss on Stellar Evolution; IAU Colloquium no. 5 C. Chiosi,R. Stalio Book 1981 D. Reidel Publishing Company, Dordrecht, Holl