LOGIN TO YOUR ACCOUNT

Username
Password
Remember Me
Or use your Academic/Social account:

CREATE AN ACCOUNT

Or use your Academic/Social account:

Congratulations!

You have just completed your registration at OpenAire.

Before you can login to the site, you will need to activate your account. An e-mail will be sent to you with the proper instructions.

Important!

Please note that this site is currently undergoing Beta testing.
Any new content you create is not guaranteed to be present to the final version of the site upon release.

Thank you for your patience,
OpenAire Dev Team.

Close This Message

CREATE AN ACCOUNT

Name:
Username:
Password:
Verify Password:
E-mail:
Verify E-mail:
*All Fields Are Required.
Please Verify You Are Human:
fbtwitterlinkedinvimeoflicker grey 14rssslideshare1
Woan, G. (2005)
Publisher: SPIE
Languages: English
Types: Other
Subjects: QB

Classified by OpenAIRE into

arxiv: Astrophysics::High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology
Identifiers:doi:10.1117/12.550057
Recent advances in gravitational wave detectors mean that we can start to make astrophysically important\ud statements about the physics of neutron stars based on observed upper limits to their gravitational luminosity.\ud Here we consider statements we can already make about a selection of known radio pulsars, based on data from\ud the LIGO and GEO600 detectors, and look forward to what could be learned from the first detections.

Share - Bookmark

Download from

Cite this article