Skip to main content Accessibility help

We use cookies to distinguish you from other users and to provide you with a better experience on our websites. Close this message to accept cookies or find out how to manage your cookie settings.

Close cookie message
×
Home
  • Home
EnglishFrançais
Symposium - International Astronomical Union Symposium - International Astronomical Union

Article contents

Far-ultraviolet Emission from Supernova Remnant Shocks

Published online by Cambridge University Press:  25 May 2016

R. Sankrit ,
W. P. Blair  and
Fuse Snr Team
R. Sankrit
Affiliation:
Johns Hopkins University, 3400 N. Charles St., Baltimore, MD 21218, U.S.A.
W. P. Blair
Affiliation:
Johns Hopkins University, 3400 N. Charles St., Baltimore, MD 21218, U.S.A.
Fuse Snr Team
Affiliation:
JHU, Princeton, GSFC, IAP, UC Berkeley
Save pdf (0.24 mb)

Abstract

Supernova remnant shocks produce a rich spectrum of lines in the ultraviolet. Among these are important diagnostic resonance lines of O VI, C III, and N III which lie in the bandpass observable with the recently launched Far Ultraviolet Spectroscopic Explorer. We present an overview of a PI program to observe several supernova remnants using this new telescope.

Type
Part II: Posters
Information
Symposium - International Astronomical Union , Volume 195: Highly Energetic Physical Processes and Mechanisms , 2000 , pp. 425 - 426
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

Blair, W. P., Sankrit, R., Raymond, J. C., & Long, K. S. 1999, AJ, 118, 942.CrossRefGoogle Scholar
Levenson, N. A., Graham, J. R., Keller, L. D., & Richter, M. J. 1998, ApJS, 118, 541.CrossRefGoogle Scholar
Sankrit, R. & Hester, J. J. 1997, ApJ, 491, 796.CrossRefGoogle Scholar

Full text views

Full text views reflects PDF downloads, PDFs sent to Google Drive, Dropbox and Kindle and HTML full text views.

Total number of HTML views: 0
Total number of PDF views: 45 *
View data table for this chart

* Views captured on Cambridge Core between September 2016 - 21st January 2021. This data will be updated every 24 hours.

Access
Hostname: page-component-76cb886bbf-2crfx Total loading time: 0.626 Render date: 2021-01-21T03:10:23.731Z Query parameters: { "hasAccess": "1", "openAccess": "0", "isLogged": "0", "lang": "en" } Feature Flags: { "shouldUseShareProductTool": true, "shouldUseHypothesis": true, "isUnsiloEnabled": true, "metricsAbstractViews": false, "figures": false, "newCiteModal": false }

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.

Far-ultraviolet Emission from Supernova Remnant Shocks
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.

Far-ultraviolet Emission from Supernova Remnant Shocks
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.

Far-ultraviolet Emission from Supernova Remnant Shocks
Available formats
×
×

Reply to: Submit a response

Your details

Conflicting interests

Do you have any conflicting interests? *