“EARLY” AND “LATE” RUNAWAY STARS IN THE ORION BN/KL REGION
We review the dynamical origin of the high proper motion BN–I–n radio sources in the Orion BN/KL region, emphasizing the apparent contradiction between the ages of the sources and the dynamical co llapse time. We show that further generations of runaway stars can be produced after the initial coll a...
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| Pubblicato in: | Revista Mexicana de Astronomía y Astrofísica |
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| Autore principale: | |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Universidad Nacional Autónoma de México
2015
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| Soggetti: | |
| Accesso online: | https://www.redalyc.org/articulo.oa?id=57150514010 |
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