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23 April 2024 |
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Interactions between a Bright YSO and the MSX Infrared-Dark Cloud G79.3+0.3: An Early Stage of Triggered Star Formation? | | R. O. Redman
; P. A. Feldman
; F. Wyrowski
; S. Cote
; S. J. Carey
; M. P. Egan
; | | Date: |
6 Dec 2002 | | Journal: | Astrophys.J. 586 (2003) 1127-1135 | | Subject: | astro-ph | | Affiliation: | NRC/Hia), P. A. Feldman (NRC/Hia), F. Wyrowski (MPIfR), S. Cote (NRC/Hia), S. J. Carey (Caltech), M. P. Egan (AFRL | | Abstract: | Millimeter and mid-infrared observations have been made of the dense clumps of dust and gas and of young stellar objects (YSOs) associated with the bright, compact submillimeter source G79.3+0.3 P1 in the relatively nearby MSX infrared-dark cloud G79.3+0.3. The Gemini mid-infrared observations reported here indicate the presence of three YSOs within the cloud. BIMA 3 mm continuum observations show that the brightest of the YSOs is likely to be a Herbig Ae/Be star. High-angular-resolution molecular-line observations suggest that a wind from this star may be triggering collapse in the adjacent molecular cloud. The submillimeter source G79.3+0.3 P1 itself does not contain infrared sources and may represent an earlier stage of star formation. | | Source: | arXiv, astro-ph/0212172 | | Services: | Forum | Review | PDF | Favorites | |
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