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arXiv 1601.05913astro-ph.SR
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掠食包络演化过程中的中间光度光学瞬变(GEE)

Intermediate luminosity optical transients during the grazing envelope evolution (GEE)

Noam Soker

摘要:

通过比较光子扩散时间与气体流出时间,我认为,在掠食包络演化(GEE)的射流所携带的能量的很大一部分可能会在辐射结束,从而导致中间光度光学瞬态(COST)。在GEE中,一颗环绕较大主星外围的伴星通过一个吸积盘吸积物质,并发射出喷流,有效地将次级恒星附近的包层气体清除。在伴星质量吸积率很高的情况下,喷流携带的能量超过了喷射质量的复合能,而当主星是巨星时,这种能量也超过了双星系统的引力结合能。一些未来的巨星暴可能更好地解释了GEE比合并和共同的信封演变没有喷流。

英文摘要:

By comparing photon diffusion time with gas outflow time, I argue that a large fraction of the energy carried by the jets during the grazing envelope evolution (GEE) might end in radiation, hence leading to an intermediate luminosity optical transient (ILOT). In the GEE a companion orbiting near the outskirts of the larger primary star accretes mass through an accretion disk, and launches jets that efficiently remove the envelope gas from the vicinity of the secondary star. In cases of high mass accretion rates onto the stellar companion the energy carried by the jets surpass the recombination energy from the ejected mass, and when the primary star is a giant this energy surpasses also the gravitational binding energy of the binary system. Some future ILOTs of giant stars might be better explained by the GEE than by merger and common envelope evolution without jets.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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