CaltechAUTHORS
  A Caltech Library Service

^(13)CH_3OH in OMC-1

Blake, Geoffrey A. and Sutton, E. C. and Masson, C. R. and Phillips, T. G. and Herbst, Eric and Plummer, Grant M. and De Lucia, Frank C. (1984) ^(13)CH_3OH in OMC-1. Astrophysical Journal, 286 . pp. 586-590. ISSN 0004-637X. doi:10.1086/162633. https://resolver.caltech.edu/CaltechAUTHORS:20120912-070230231

[img]
Preview
PDF - Published Version
See Usage Policy.

691kB

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20120912-070230231

Abstract

We report the identification of several previously unidentified or misidentified lines toward OMC-1 as components the J = 5 → 4 α-type band of ^(13)CH_30H, deduced by combining accurate laboratory spectroscopy with sensitive broad-band astronomical line searches. An LTE fit to the data yields a rotational temperature of T_(rot)~ 120 K and a ^(13)CH_30H column density of ~1.3 x 10^(15) cm^(-2), averaged over a 30" beam. A ^(12)C/^(13)C ratio of ~30 is derived. The assignment of the feature at 236063 MHz to the blended K = ±2 E transitions of ^(13)CH_30H, rather than to CO^+, removes a major discrepancy between observation and the predictions of ion-molecule chemical models of dense interstellar clouds.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/162633DOIArticle
http://adsabs.harvard.edu/abs/1984ApJ...286..586BPublisherArticle
ORCID:
AuthorORCID
Blake, Geoffrey A.0000-0003-0787-1610
Additional Information:© 1984 American Astronomical Society. Provided by the NASA Astrophysics Data System. Received 1984 April 3; accepted 1984 June 4. Single dish millimeter-wave astronomy at the Owens Valley Radio Observatory is supported by NSF grant AST 82-14693.The authors would also like to thank R. E. Miller of AT & T Bell Laboratories, Murray Hill, for supplying the SIS junctions used in this work. E. H., G. M. P., and F. C. D. L. acknowledge support from NASA via grant NAGW-189. E. H. also wishes to acknowledge the support of the NSF via grant AST 83-12270 for his theoretical program.
Group:UNSPECIFIED, Division of Geological and Planetary Sciences
Funders:
Funding AgencyGrant Number
NSFAST 82-14693
NASANAGW-189
NSFAST 83-12270
Subject Keywords:interstellar: abundances; interstellar: molecules; line identifications
DOI:10.1086/162633
Record Number:CaltechAUTHORS:20120912-070230231
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20120912-070230231
Official Citation:C-13H3OH in OMC-1 Blake, G. A., Sutton, E. C., Masson, C. R., Phillips, T. G., Herbst, E., Plummer, G. M., , Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 286, Nov. 15, 1984, p. 586-590.
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:34011
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:12 Sep 2012 15:02
Last Modified:09 Nov 2021 23:06

Repository Staff Only: item control page