Multiband optical and infrared photometry of CH Cygni

Details Multiband optical and infrared photometry of CH Cygni Multiband optical and infrared photometry of CH Cygni

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982sval....8..389t&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 8, Dec. 1982, p. 722-724) Soviet Astronomy Letters (ISSN 0360-0327), vol. 8, Nov.-Dec.

Astronomy and Astrophysics

Astronomy

2

Giant Stars, Infrared Photometry, Infrared Spectra, M Stars, Optical Emission Spectroscopy, Stellar Spectrophotometry, Black Body Radiation, Interstellar Extinction, Light Curve, Spectral Energy Distribution, Spectrum Analysis, Stellar Magnitude, Ubv Spectra

Scientific paper

Preliminary analysis of UBVRJHKLMNQ photometry of CH Cyg during 1978-1982 indicates that when this systemn is in its active state the infrared radiation of the cool (M6 III) component undergoes semiregular fluctuations coinciding in period and phase with the quiescent variability. An improved value is obtained for the distance: 310 + or - 50 pc. From 1978 to March 1982, CH Cyg brightened optically by approximately 2.5 m.

Affiliated with

Also associated with

No associations

Rating

Multiband optical and infrared photometry of CH Cygni 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 Multiband optical and infrared photometry of CH Cygni, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Multiband optical and infrared photometry of CH Cygni will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-932409