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Nascent bipolar outflows associated with the first hydrostatic core candidates Barnard 1b-N and 1b-S()
In the theory of star formation, the first hydrostatic core (FHSC) phase is a critical step in which a condensed object emerges from a prestellar core. This step lasts about one thousand years, a very short time compared with the lifetime of prestellar cores, and therefore is hard to detect unambigu...
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| Yayımlandı: | Astron Astrophys |
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| Asıl Yazarlar: | , , , , , |
| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
2015
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| Konular: | |
| Online Erişim: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7116309/ https://ncbi.nlm.nih.gov/pubmed/33154595 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1051/0004-6361/201525777 |
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