CONVERGENT FLOWS AND LOW-VELOCITY SHOCKS IN DR21(OH)

Journal Article · Mon Oct 10 04:00:00 EDT 2011 · Astrophysical Journal Letters

DOI:https://doi.org/10.1088/2041-8205/740/1/L5· OSTI ID:21565410

Csengeri, T ^[1]; Bontemps, S ^[2]; Schneider, N; Motte, F ^[3]; Gueth, F ^[4]

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1. Max Planck Institute for Radioastronomy, Auf dem Huegel 69, 53121 Bonn (Germany)
2. OASU/LAB-UMR5804, CNRS, Universite Bordeaux 1, 33270 Floirac (France)
3. Laboratoire AIM Paris Saclay, CEA-INSU/CNRS-Universite Paris Diderot, IRFU/SAp CEA-Saclay, 91191 Gif-sur-Yvette (France)
4. IRAM, 300 rue de la piscine, 38406, Saint Martin d'Heres (France)

DR21(OH) is a pc-scale massive, {approx}7000 M{sub sun} clump hosting three massive dense cores (MDCs) at an early stage of their evolution. We present a high angular resolution mosaic, covering {approx}70'' x 100'', with the IRAM Plateau de Bure Interferometer at 3 mm to trace the dust continuum emission and the N{sub 2}H{sup +} (J = 1-0) and CH{sub 3}CN (J = 5-4) molecular emission. The cold, dense gas traced by the compact emission in N{sub 2}H{sup +} is associated with the three MDCs and shows several velocity components toward each MDC. These velocity components reveal local shears in the velocity fields which are best interpreted as convergent flows. Moreover, we report the detection of weak extended emission from CH{sub 3}CN at the position of the N{sub 2}H{sup +} velocity shears. We propose that this extended CH{sub 3}CN emission is tracing warm gas associated with the low-velocity shocks expected at the location of convergence of the flows where velocity shears are observed. This is the first detection of low-velocity shocks associated with small (subparsec) scale convergent flows which are proposed to be at the origin of the densest structures and of the formation of (high-mass) stars. In addition, we propose that MDCs may be active sites of star formation for more than a crossing time as they continuously receive material from larger scale flows as suggested by the global picture of dynamical, gravity-driven evolution of massive clumps which is favored by the present observations.

• OSTI ID: 21565410
• Journal Information: Astrophysical Journal Letters, Journal Name: Astrophysical Journal Letters Journal Issue: 1 Vol. 740; ISSN 2041-8205
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
ACETONITRILE
EMISSION
EVOLUTION
NITRILES
ORGANIC COMPOUNDS
ORGANIC NITROGEN COMPOUNDS
SHOCK WAVES
STAR EVOLUTION
VELOCITY