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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...

Deskribapen osoa

Gorde:
Xehetasun bibliografikoak
Egile Nagusiak: Rodríguez, L F, Mirabel, I F
Formatua: Artigo
Hizkuntza:Inglês
Argitaratua: 1995
Gaiak:
Sarrera elektronikoa:https://ncbi.nlm.nih.gov/pmc/articles/PMC40407/
https://ncbi.nlm.nih.gov/pubmed/11607605
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