Deharveng, L., Lefloch, B., Zavagno, A., Caplan, J., Whitworth, Anthony Peter ![]() |
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Abstract
We present millimetre-line imaging of the Galactic H II region Sh 104. We show that it is surrounded by a ring of molecular gas and dust. Four large molecular condensations are regularly spaced around the ring. These condensations are themselves fragmented and contain several massive dense cores. A deeply embedded cluster is observed in the near IR towards the largest condensation. It contains at least one massive star ionizing an ultra-compact H II region. The Sh 104 region is a good illustration of the "collect and collapse" model for star formation triggered by the expansion of an H II region.
Item Type: | Article |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QB Astronomy |
Uncontrolled Keywords: | stars: formation; stars: early-type; ISM: H II regions; ISM: individual: Sh2-104 |
Additional Information: | Pdf uploaded in accordance with publisher's policy at http://www.sherpa.ac.uk/romeo/issn/0004-6361/ (accessed 17/04/2014) |
Publisher: | EDP sciences |
ISSN: | 0004-6361 |
Date of First Compliant Deposit: | 30 March 2016 |
Last Modified: | 16 May 2023 11:59 |
URI: | https://orca.cardiff.ac.uk/id/eprint/47410 |
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