Skip to main content Accessibility help
×
Home
Hostname: page-component-59df476f6b-6nvld Total loading time: 0.187 Render date: 2021-05-18T04:58:52.222Z Has data issue: true Feature Flags: { "shouldUseShareProductTool": true, "shouldUseHypothesis": true, "isUnsiloEnabled": true, "metricsAbstractViews": false, "figures": true, "newCiteModal": false, "newCitedByModal": true, "newEcommerce": true }

Cold HI Gas in the M17SW Giant Molecular Cloud

Published online by Cambridge University Press:  25 April 2016

F. Sato
Affiliation:
Tokyo Gakugei University, Loganei, Tokyo, Japan
J. B. Whiteoak
Affiliation:
Australia Telescope National Facility, PO Box 76 Epping, NSW 2121
R. E. Otrupcek
Affiliation:
Australia Telescope National Facility, PO Box 76 Epping, NSW 2121
T. Tokushige
Affiliation:
Tokyo Gakugei University, Koganei, Tokyo, Japan

Abstract

The cold HI cloud in the region of the M17SW giant molecular cloud comprises three major fragments with a mean size of ~ 30 pc. Their overall distribution is rather similar to that of CO gas, but one of the fragments does not seem to have a molecular counterpart. It is shown that such a cloud is also a future site of star formation.

Type
Galactic and Stellar
Copyright
Copyright © Astronomical Society of Australia 1991

Access options

Get access to the full version of this content by using one of the access options below.

References

Elmegreen, B. G. et al., 1979, Astrophys. J., 230, 415.CrossRefGoogle Scholar
Hasegawa, T., Sato, F. and Fukui, Y., 1983, Astron. J., 88, 658.CrossRefGoogle Scholar
Jaffe, D. T. et al, 1982, Astrophys. J., 252, 601.CrossRefGoogle Scholar
Sato, F., 1990, Astron. J., 99, 1897.CrossRefGoogle Scholar
Sato, F. and Fukui, Y., 1978, Astron. J., 83, 1607.CrossRefGoogle Scholar
Sato, F. et al., 1980, IAU Symp. No. 87, 187.Google Scholar
Sato, F., Whiteoalc, J.B., Otrupcek, R.E. and Tokushige, T., 1991, this volume.Google Scholar

Send article to Kindle

To send this article to your Kindle, first ensure no-reply@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about sending to your Kindle. Find out more about sending to your Kindle.

Note you can select to send to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be sent to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

Cold HI Gas in the M17SW Giant Molecular Cloud
Available formats
×

Send article to Dropbox

To send this article to your Dropbox account, please select one or more formats and confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your <service> account. Find out more about sending content to Dropbox.

Cold HI Gas in the M17SW Giant Molecular Cloud
Available formats
×

Send article to Google Drive

To send this article to your Google Drive account, please select one or more formats and confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your <service> account. Find out more about sending content to Google Drive.

Cold HI Gas in the M17SW Giant Molecular Cloud
Available formats
×
×

Reply to: Submit a response


Your details


Conflicting interests

Do you have any conflicting interests? *