A young giant molecular cloud formed at the interface of two colliding supershells

Observations meet simulations

J. R. Dawson, E. Ntormousi, Y. Fukui, T. Hayakawa, K. Fierlinger

Research output: Contribution to journalArticle

14 Citations (Scopus)
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Abstract

Dense, star-forming gas is believed to form at the stagnation points of large-scale interstellar medium flows, but observational examples of this process in action are rare. We here present a giant molecular cloud (GMC) sandwiched between two colliding Milky Way supershells, which we argue shows strong evidence of having formed from material accumulated at the collision zone. Combining 12CO, 13CO, and C18O(J = 1-0) data with new high-resolution, three-dimensional hydrodynamical simulations of colliding supershells, we discuss the origin and nature of the GMC (G288.5+1.5), favoring a scenario in which the cloud was partially seeded by pre-existing denser material, but assembled into its current form by the action of the shells. This assembly includes the production of some new molecular gas. The GMC is well interpreted as non-self-gravitating, despite its high mass (), and is likely pressure confined by the colliding flows, implying that self-gravity was not a necessary ingredient for its formation. Much of the molecular gas is relatively diffuse, and the cloud as a whole shows little evidence of star formation activity, supporting a scenario in which it is young and recently formed. Drip-like formations along its lower edge may be explained by fluid dynamical instabilities in the cooled gas.

Original languageEnglish
Article number64
Pages (from-to)1-12
Number of pages12
JournalAstrophysical Journal
Volume799
Issue number1
DOIs
Publication statusPublished - 20 Jan 2015

Bibliographical note

Copyright 2015 The American Astronomical Society. First published in the Astrophysical journal, 799(1), 64, 2015. The original publication is available at http://dx.doi.org/10.1088/0004-637X/799/1/64, published by IOP Publishing. Version archived for private and non-commercial use with the permission of the author/s and according to publisher conditions. For further rights please contact the publisher.

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