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Blowout from IC 1396N: The Emergence of Herbig-Haro Flows from a Cloud Core

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Published 2003 July 15 © 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Bo Reipurth et al 2003 ApJ 593 L47 DOI 10.1086/378147

1538-4357/593/1/L47

Abstract

We have identified a major Herbig-Haro flow, HH 777, that is bursting out of the IC 1396N cometary cloud core. Near- and mid-infrared images reveal a very red object embedded in the center of the core, located on the symmetry axis of the large HH 777 flow, suggesting that this is likely the driving source. The projected separation of the working surface from the source is 0.6 pc. Additionally, 0.4 pc to the east of the source and on the flow axis, there is a faint, previously known HH object (HH 594) that may be part of the counterflow. It thus appears that we are seeing a blowout of a parsec-scale flow into the surrounding H II region. We study numerical simulations of a jet breaking out of a neutral cloud into a photoionized medium, and we reproduce the main features of the HH 777 flow.

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10.1086/378147