Skip to main content Accessibility help
×
Home
Hostname: page-component-564cf476b6-4htn5 Total loading time: 0.21 Render date: 2021-06-20T05:33:08.293Z Has data issue: true Feature Flags: { "shouldUseShareProductTool": true, "shouldUseHypothesis": true, "isUnsiloEnabled": true, "metricsAbstractViews": false, "figures": true, "newCiteModal": false, "newCitedByModal": true, "newEcommerce": true }

Detailed stellar and gaseous kinematics of M31

Published online by Cambridge University Press:  09 February 2015

Michael Opitsch
Affiliation:
Max Planck Institute for Extraterrestrial Physics, Gießenbachstr., 80748 Garching, Germany email: mopitsch@mpe.mpg.de University Observatory Munich, Scheinerstr. 1, 81679 Munich, Germany Excellence Cluster Universe, Boltzmannstr. 2, 85748 Garching, Germany
Maximilian Fabricius
Affiliation:
Max Planck Institute for Extraterrestrial Physics, Gießenbachstr., 80748 Garching, Germany email: mopitsch@mpe.mpg.de University Observatory Munich, Scheinerstr. 1, 81679 Munich, Germany
Roberto Saglia
Affiliation:
Max Planck Institute for Extraterrestrial Physics, Gießenbachstr., 80748 Garching, Germany email: mopitsch@mpe.mpg.de University Observatory Munich, Scheinerstr. 1, 81679 Munich, Germany
Ralf Bender
Affiliation:
Max Planck Institute for Extraterrestrial Physics, Gießenbachstr., 80748 Garching, Germany email: mopitsch@mpe.mpg.de University Observatory Munich, Scheinerstr. 1, 81679 Munich, Germany
Michael Williams
Affiliation:
Max Planck Institute for Extraterrestrial Physics, Gießenbachstr., 80748 Garching, Germany email: mopitsch@mpe.mpg.de Department of Astronomy, Columbia University, 550 West 120th Street, NY10027 New York, USA
Corresponding
E-mail address:
Rights & Permissions[Opens in a new window]

Abstract

We have collected optical integral field spectroscopic data for M31 with the spectrograph VIRUS-W that result in kinematic maps of unprecedented detail. These reveal the presence of two kinematically distinct gas components.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2015 

References

Cappellari, M. & Emsellem, E. 2004, PASP, 116, 138CrossRefGoogle Scholar
Courteau, S., et al. 2011, ApJ, 739, 20CrossRefGoogle Scholar
Fabricius, M. H.et al. 2008, SPIE, 7014, 234Google Scholar
Sarzi, M.et al., 2006 MNRAS, 366, 1151CrossRefGoogle Scholar
You have Access

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.

Detailed stellar and gaseous kinematics of M31
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.

Detailed stellar and gaseous kinematics of M31
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.

Detailed stellar and gaseous kinematics of M31
Available formats
×
×

Reply to: Submit a response

Please enter your response.

Your details

Please enter a valid email address.

Conflicting interests

Do you have any conflicting interests? *