Soft X-rays from the intermediate-age open cluster NGC 752.

Details Soft X-rays from the intermediate-age open cluster NGC 752. Soft X-rays from the intermediate-age open cluster NGC 752.

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...305..806b&link_type=abstract

Astronomy and Astrophysics, v.305, p.806

Astronomy and Astrophysics

Astrophysics

21

Stars: Activity, Open Clusters And Associations: Individual: Ngc 752, X-Rays: Stars

Scientific paper

A ROSAT PSPC observation of NGC 752 detects 49 sources. Seven sources are tentatively identified with optical cluster members, of which three are short-period binaries, one is a blue straggler, and one a rapid rotator. The eclipsing binary DS And - also a cluster member - is probably detected as well. The X-ray properties of these sources are similar to those of RS CVn binaries with the same absolute magnitude and colour in the galactic disk.

Affiliated with

Also associated with

No associations

Rating

Soft X-rays from the intermediate-age open cluster NGC 752. 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 Soft X-rays from the intermediate-age open cluster NGC 752., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Soft X-rays from the intermediate-age open cluster NGC 752. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-967056