Two short lived X-ray transients at high galactic latitude

Details Two short lived X-ray transients at high galactic latitude Two short lived X-ray transients at high galactic latitude

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976natur.261..564c&link_type=abstract

Nature, vol. 261, June 17, 1976, p. 564-566. Research supported by the Science Research Council.

Physics

20

Light Curve, M Stars, Transient Response, Variable Stars, X Ray Sources, Ariel Satellites, Error Analysis, Flares, Mira Variables, Position Errors

Scientific paper

Ariel V observations of two transient X-ray sources at high galactic latitudes are reported. The characteristic time scales of these sources, A0000+28 and A0353-40, are of the order of hundreds of minutes. It is found that the error box of the first source contains a Mira-type variable and that the error box of the second source contains the bright reflection nebulosity NGC 5367. Noting that this nebulosity probably has UV Ceti flare stars embedded within it, the possibility is considered that both sources are associated with flare stars.

Affiliated with

Also associated with

No associations

Rating

Two short lived X-ray transients at high galactic latitude 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 Two short lived X-ray transients at high galactic latitude, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Two short lived X-ray transients at high galactic latitude will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1784825