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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| 出版年: | Proc Natl Acad Sci U S A |
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| 主要な著者: | , |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
National Academy of Sciences
1995
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| 主題: | |
| オンライン･アクセス: | 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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