The proto-planetary nebula M1-92 and the symbiotic star MWC 560: Two evolutionary phases of the same type of object?

被引:17
作者
Arrieta, A
Torres-Peimbert, S
Georgiev, L
机构
[1] Univ Iberoamer, Dept Fis & Matemat, Mexico City 01210, DF, Mexico
[2] Natl Autonomous Univ Mexico, Inst Astron, Mexico City 04510, DF, Mexico
关键词
binaries : symbiotic; ISM : jets and outflows; planetary nebulae : individual (M1-92); stars : AGB and post-AGB; stars : individual (MWC 560);
D O I
10.1086/428391
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Important similarities between the objects M1-92, a proto - planetary nebula of bipolar morphology, and MWC 560, a symbiotic star with a jet, have been found. A brief review of the previous studies for both objects is presented for the purpose of proposing mechanisms that best explain these similarities, since up to now both objects have been studied independently. From the comparison of the spectra of both objects, the existence of a jet is confirmed for the proto - planetary nebula M1-92, as well as its binary nature and the existence of a circumnuclear disk. Finally, an evolutionary sequence is proposed for the two objects where M1-92 is similar to 900 yr more evolved than MWC 560.
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页码:252 / 268
页数:17
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