Protostellar clusters in intermediate mass (IM) star forming regions
Context.The transition between the low density groups of T Tauri stars and the high density clusters around massive stars occurs in the intermediate-mass (IM) range ($M_*\sim2{-}8~M_\odot$). High spatial resolution studies of IM young stellar objects (YSO) can provide important clues to understand t...
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Published in | Astronomy and astrophysics (Berlin) Vol. 468; no. 3; pp. L37 - L40 |
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Main Authors | , , , , , , , |
Format | Journal Article |
Language | English |
Published |
EDP Sciences
01.06.2007
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Subjects | |
Online Access | Get full text |
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Summary: | Context.The transition between the low density groups of T Tauri stars and the high density clusters around massive stars occurs in the intermediate-mass (IM) range ($M_*\sim2{-}8~M_\odot$). High spatial resolution studies of IM young stellar objects (YSO) can provide important clues to understand the clustering in massive star forming regions. Aims.Our aim is to search for clustering in IM Class 0 protostars. The high spatial resolution and sensitivity provided by the new A configuration of the Plateau de Bure Interferometer (PdBI) allow us to study the clustering in these nearby objects. Methods.We have imaged three IM Class 0 protostars (Serpens-FIRS 1, IC 1396 N, CB 3) in the continuum at 3.3 and 1.3 mm using the PdBI. The sources have been selected with different luminosity to investigate the dependence of the clustering process on the luminosity of the source. Results.Only one millimeter (mm) source is detected towards the low luminosity source Serpens-FIRS 1. Towards CB 3 and IC1396 N, we detect two compact sources separated by ~0.05 pc. The 1.3 mm image of IC 1396 N, which provides the highest spatial resolution, reveal that one of these cores is splitted in, at least, three individual sources. |
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Bibliography: | ark:/67375/80W-9CZSNJLR-J istex:50D46C38665EFA8DA1161FBF939AD573D789C8E2 publisher-ID:aa7297-07 other:2007A%26A...468L..37F ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
ISSN: | 0004-6361 1432-0746 1432-0756 |
DOI: | 10.1051/0004-6361:20077297 |