Cold water vapor in the Barnard 5 molecular cloud

10Citations
Citations of this article
11Readers
Mendeley users who have this article in their library.

Abstract

After more than 30 yr of investigations, the nature of gas-grain interactions at low temperatures remains an unresolved issue in astrochemistry. Water ice is the dominant ice found in cold molecular clouds; however, there is only one region where cold (10 K) water vapor has been detected - L1544. This study aims to shed light on ice desorption mechanisms under cold cloud conditions by expanding the sample. The clumpy distribution of methanol in dark clouds testifies to transient desorption processes at work - likely to also disrupt water ice mantles. Therefore, the Herschel HIFI instrument was used to search for cold water in a small sample of prominent methanol emission peaks. We report detections of the ground-state transition of o-H2O (J = 110-101) at 556.9360 GHz toward two positions in the cold molecular cloud, Barnard 5. The relative abundances of methanol and water gas support a desorption mechanism which disrupts the outer ice mantle layers, rather than causing complete mantle removal. © 2014. The American Astronomical Society. All rights reserved.

Cite

CITATION STYLE

APA

Wirström, E. S., Charnley, S. B., Persson, C. M., Buckle, J. V., Cordiner, M. A., & Takakuwa, S. (2014). Cold water vapor in the Barnard 5 molecular cloud. Astrophysical Journal Letters, 788(2). https://doi.org/10.1088/2041-8205/788/2/L32

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free