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Title: COEVAL INTERMEDIATE-MASS STAR FORMATION IN N4W

Journal Article · · Astrophysical Journal
; ; ;  [1]; ;  [2]
  1. Purple Mountain Observatory and Key Laboratory for Radio Astronomy, Chinese Academy of Sciences, 2 West Beijing Road, 210008 Nanjing (China)
  2. Department of Astronomy, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan)

Protostars are mostly found in star-forming regions, where the natal molecular gas still remains. At about 5{sup ′} west of the molecular bubble N4, N4W is identified as a star-forming clump hosting three Class II (IRS 1–3), and one Class I (IRS 4) young stellar objects (YSOs), as well as a submillimeter source SMM1. The near-IR polarization imaging data of N4W reveal two infrared reflection nebulae close to each other, which are in favor of the outflows of IRS 1 and IRS 2. The bipolar mid-IR emission centered on IRS 4 and the arc-like molecular gas shell are lying on the same axis, indicating a bipolar molecular outflow from IRS 4. There are two dust temperature distributions in N4W. The warmer one is widely distributed and has a temperature of T{sub d}≳28 K, with the colder one being from the embedded compact submillimeter source SMM1. N4W’s mass is estimated to be ∼2.5×10{sup 3} M{sub ⊙}, and the mass of SMM1 is ∼5.5×10{sup 2} M{sub ⊙} at T{sub d}=15 K, calculated from the CO 1 − 0 emission and 870 μm dust continuum emission, respectively. Based on the estimates of the bolometric luminosity of IRS 1–4, these four sources are intermediate-mass YSOs at least. SMM1 is gravitationally bound, and is capable of forming intermediate-mass stars or even possibly massive stars. The co-existence of the IR bright YSOs and the submillimeter source represents potential sequential star formation processes separated by ∼0.5 Myr in N4W. This small age spread implies that the intermediate-mass star formation processes happening in N4W are almost coeval.

OSTI ID:
22862948
Journal Information:
Astrophysical Journal, Vol. 822, Issue 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
Country of Publication:
United States
Language:
English