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...
Tallennettuna:
| Julkaisussa: | Proc Natl Acad Sci U S A |
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| Päätekijät: | , |
| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
National Academy of Sciences
1995
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| Aiheet: | |
| Linkit: | 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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