Discovery of flare activity on BD+66 deg 34 /= Gliese 22A/

Details Discovery of flare activity on BD+66 deg 34 /= Gliese 22A/ Discovery of flare activity on BD+66 deg 34 /= Gliese 22A/

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....41..113p&link_type=abstract

Astronomy and Astrophysics, vol. 41, no. 1, June 1975, p. 113.

Astronomy and Astrophysics

Astrophysics

6

Dwarf Stars, Flares, Light Curve, M Stars, Stellar Luminosity, Astronomical Photometry, Companion Stars, Star Distribution, Stellar Spectra, Triple Stars, Variable Stars

Scientific paper

The triple star system BD+66 deg 34 consists of the non-emission line M dwarf Gliese 22B and the brighter component Gliese 22A with its unseen companion. The spectrum of Gliese 22A is classified as dM 2.5e. Andersen and Pettersen (1975) have proposed that Gliese 22A is a UV Cet-type flare star. The discovery of flare activity on one of the components of this system is reported.

Affiliated with

Also associated with

No associations

Rating

Discovery of flare activity on BD+66 deg 34 /= Gliese 22A/ 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 Discovery of flare activity on BD+66 deg 34 /= Gliese 22A/, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Discovery of flare activity on BD+66 deg 34 /= Gliese 22A/ will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-747949