The Infrared Variability and Nature of Symbiotic Stars - Part Four - Rx-Puppis

Details The Infrared Variability and Nature of Symbiotic Stars - Part Four - Rx-Puppis The Infrared Variability and Nature of Symbiotic Stars - Part Four - Rx-Puppis

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.203..363w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 203, P. 363, 1983

Astronomy and Astrophysics

Astronomy

23

Scientific paper

Extensive JHKL observations for the years 1972-82 are tabulated. A Mira variable of period 580 days is present in the system which has a distance of 3.0 kpc. The mean J brightness of thye system was constant from 1975 to 1979 but then decreased as did the V brightness. Some or all of this decrease may be due to a reduction in free-free and free-bound emission at both wavelengths. Alternatively there may be variable dust obscuration. The L magnitudes show that the flux from heated dust in the system increased steadily from 1975 until at least 1979 and less certainly until the present time.

Affiliated with

Also associated with

No associations

Rating

The Infrared Variability and Nature of Symbiotic Stars - Part Four - Rx-Puppis 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 The Infrared Variability and Nature of Symbiotic Stars - Part Four - Rx-Puppis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Infrared Variability and Nature of Symbiotic Stars - Part Four - Rx-Puppis will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1235355