Multicolour photometry of the M0V+M5V eclipsing binary V405 And

Details Multicolour photometry of the M0V+M5V eclipsing binary V405 And Multicolour photometry of the M0V+M5V eclipsing binary V405 And

2008-09-29

arxiv.org/abs/0809.5029v2

AIP Conf.Proc.1094:812-815,2009

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures, 1 table, proceedings of Cool Stars 15, St Andrews, July 2008, to be published in the Conference Proceeding

Scientific paper

10.1063/1.3099240

We present multicolour photometry and modelling of the active eclipsing binary star V405 And. The components of 0.2 and 0.5 solar masses are just below and above the theoretical limit of the full convection, that is thought to be around 0.3 solar mass. The light curves are compositions of constant and variable features: the distorted shape of the components (about 25%), a small eclipse, and mainly of spots (about 75%) and flares.

Affiliated with

Also associated with

No associations

Rating

Multicolour photometry of the M0V+M5V eclipsing binary V405 And 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 Multicolour photometry of the M0V+M5V eclipsing binary V405 And, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Multicolour photometry of the M0V+M5V eclipsing binary V405 And will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-49750