Search for CO Outflows toward a Sample of 69 High-Mass Protostellar Candidates. II. Outflow Properties

By Qizhou Zhang, T. Hunter, J. Brand, Sridharan T. K., R. Cesaroni, Sergio Molinari, Junzhi Wang, M. Kramer. 2005

224 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/3553376255977e864ef03a2cba2e52e92a79f3e2

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In Astronomy and Astrophysics

1. Mark R. Krumholz
2. Ralf Klessen
3. N. Evans II
4. Christoph Federrath
5. Y. Shirley
6. S. Glover
7. Tom Abel
8. T. Hosokawa

In Spectroscopy

1. N. Evans II
2. Mark R. Krumholz
3. Y. Shirley
4. P. V. Vanden Bout
5. Jingwen Wu
6. C. Knez
7. Th. Henning
8. P. Solomon

Citations in the corpus

• The evolution of the spectral energy distribution in massive young stellar objects (2008, background): “…even one order of magnitude higher are usually postulated based on the inferred mass loss rates measured for molecular outflows in high-mass YSOs (Zhang et al. 2001, 2005); under these conditions the arrival onto the ZAMS can be deferred to higher masses provided the required ever higher…”
• Hierarchical fragmentation and differential star formation in the Galactic ‘Snake’: infrared dark cloud G11.11−0.12 (2014, background): “Compared with outflow P1-SMA1, the P6 outflows are slightly less energetic but are still comparable with other high-mass outflows (Beuther et al. 2002; Zhang et al. 2005).”
• OUTFLOW FEEDBACK REGULATED MASSIVE STAR FORMATION IN PARSEC-SCALE CLUSTER-FORMING CLUMPS (2009, background): “…consistent with the dynamical times estimated for massive molecular outflows (which are presumably driven by rapid mass accretion during the main accretion phase, as in the case of low-mass stars; e.g., Bontemps et al. 1996), which are typically of order 105 yr or less (e.g., Zhang et al. 2005).”
• EVOLUTION OF MASSIVE PROTOSTARS WITH HIGH ACCRETION RATES (2008, background): “Molecular outflows are also ubiquitous in high-mass star-forming regions, and estimated high mass outflow rates also suggest high accretion rates 1 (e.g., Beuther et al. 2002; Zhang et al. 2005).”
• THE PROPERTIES OF MASSIVE, DENSE CLUMPS: MAPPING SURVEYS OF HCN AND CS (2010, methodology): “To extend the sample towards lower luminosities for the study of L′HCN -LIR correlation, we selected 14 IRAS sources from outflow surveys (Zhang et al. 2005; Wu et al. 2004) and a few lower mass clumps from other publications.”
• Connecting Dense Gas Tracers of Star Formation in our Galaxy to High-z Star Formation (2005, methodology): “To extend the sample towards lower luminosities, we selected 14 IRAS sources from outflow surveys (Zhang et al. 2005; Wu et al. 2004) and a few from other publications.”