Grs 1915+105: a superluminal source in the Galaxy.

We present the results of additional observations of the high energy source GRS 1915+105, which produces ejecta with apparent superluminal motions. The observations reported here were carried out with the Very Large Array at 3.5 cm and 20 cm. The 3.5-cm observations made during 1994 May allowed us t...

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發表在:	Proc Natl Acad Sci U S A
Principais autores:	Rodríguez, L F, Mirabel, I F
格式:	Artigo
語言:	Inglês
出版:	National Academy of Sciences 1995
主題:	Research Article
在線閱讀:	https://ncbi.nlm.nih.govhttps://pmc.ncbi.nlm.nih.gov/articles/PMC40407/ https://ncbi.nlm.nih.govhttps://pubmed.ncbi.nlm.nih.gov/11607605/ https://ncbi.nlm.nih.govhttps://doi.org/10.1073/pnas.92.25.11390
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