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Chemical segregation in the young protostars Barnard 1b-N and S Evidence of pseudo-disk rotation in Barnard 1b-S⋆
The extremely young Class 0 object B1b-S and the first hydrostatic core (FSHC) candidate, B1b-N, provide a unique opportunity to study the chemical changes produced in the elusive transition from the prestellar core to the protostellar phase. We present 40”×70” images of Barnard 1b in the (13)CO 1→0...
Tallennettuna:
| Julkaisussa: | Astron Astrophys |
|---|---|
| Päätekijät: | , , , , , , , , , |
| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
2017
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| Aiheet: | |
| Linkit: | https://ncbi.nlm.nih.gov/pmc/articles/PMC5662144/ https://ncbi.nlm.nih.gov/pubmed/29093600 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1051/0004-6361/201730963 |
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