MOLECULAR OUTFLOWS FROM THE PROTOCLUSTER SERPENS SOUTH

Journal Article · Sat Aug 20 04:00:00 EDT 2011 · Astrophysical Journal

DOI:https://doi.org/10.1088/0004-637X/737/2/56· OSTI ID:21579956

Nakamura, Fumitaka; Higuchi, Aya ^[1]; Sugitani, Kohji ^[2]; Shimajiri, Yoshito; Kawabe, Ryohei ^[3]; Tsukagoshi, Takashi ^[4]; Nishiyama, Shogo ^[5]; Takami, Michihiro; Karr, Jennifer L ^[6]; Gutermuth, Robert A; Wilson, Grant ^[7]

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1. National Astronomical Observatory, Mitaka, Tokyo 181-8588 (Japan)
2. Graduate School of Natural Sciences, Nagoya City University, Mizuho-ku, Nagoya 467-8501 (Japan)
3. Nobeyama Radio Observatory, Nobeyama, Minamimaki, Minamisaku, Nagano 384-1305 (Japan)
4. Department of Astronomy, School of Science, University of Tokyo, Bunkyo, Tokyo 113-0033 (Japan)
5. Department of Astronomy, Kyoto University, Sakyo-ku, Kyoto 606-8502 (Japan)
6. Academia Sinica Institute of Astronomy and Astrophysics, P.O. Box 23-141, Taipei 106, Taiwan (China)
7. Department of Astronomy, University of Massachusetts, Amherst, MA 01003 (United States)

We present the results of CO (J = 3-2) and HCO{sup +} (J = 4-3) mapping observations toward a nearby embedded cluster, Serpens South, using the ASTE 10 m telescope. Our CO (J = 3-2) map reveals that many outflows are crowded in the dense cluster-forming clump that can be recognized as an HCO{sup +} clump with a size of {approx}0.2 pc and mass of {approx}80 M{sub sun}. The clump contains several subfragments with sizes of {approx}0.05 pc. By comparing the CO (J = 3-2) map with the 1.1 mm dust continuum image taken by AzTEC on ASTE, we find that the spatial extents of the outflow lobes are sometimes anti-correlated with the distribution of the dense gas, and some of the outflow lobes apparently collide with the dense gas. The total outflow mass, momentum, and energy are estimated to be 0.6 M{sub sun}, 8 M{sub sun} km s{sup -1}, and 64 M{sub sun} km{sup 2} s{sup -2}, respectively. The energy injection rate due to the outflows is comparable to the turbulence dissipation rate in the clump, implying that the protostellar outflows can maintain the supersonic turbulence in this region. The total outflow energy seems only about 10% of the clump gravitational energy. We conclude that the current outflow activity is not enough to destroy the whole cluster-forming clump, and therefore star formation is likely to continue for several or many local dynamical times.

• OSTI ID: 21579956
• Journal Information: Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 2 Vol. 737; ISSN ASJOAB; ISSN 0004-637X
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
CARBON COMPOUNDS
CARBON MONOXIDE
CARBON OXIDES
CHALCOGENIDES
DUSTS
MAPPING
MASS
OXIDES
OXYGEN COMPOUNDS
STAR CLUSTERS
TURBULENCE