Finding Stellar Variables with Far-Ulatraviolet Photometry: NGC 1851

Details Finding Stellar Variables with Far-Ulatraviolet Photometry: NGC 1851 Finding Stellar Variables with Far-Ulatraviolet Photometry: NGC 1851

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21541705z&link_type=abstract

American Astronomical Society, AAS Meeting #215, #417.05; Bulletin of the American Astronomical Society, Vol. 42, p.271

Astronomy and Astrophysics

Astronomy

Scientific paper

The use of time resolved far-ultraviolet photometry is very efficient in
discovering variable sources. We show that Ultra-compact X-ray sources,
cataclysmic variables, RR Lyrae and blue stragglers are easily found in
the cores of globular clusters. We used the solar blind channel of the
Advanced Camera for Surveys on the Hubble Space Telescope.

Affiliated with

Also associated with

No associations

Rating

Finding Stellar Variables with Far-Ulatraviolet Photometry: NGC 1851 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Finding Stellar Variables with Far-Ulatraviolet Photometry: NGC 1851, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Finding Stellar Variables with Far-Ulatraviolet Photometry: NGC 1851 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-966640