MOST Satellite Photometry of Eclipsing Binaries

Details MOST Satellite Photometry of Eclipsing Binaries MOST Satellite Photometry of Eclipsing Binaries

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..435...39p&link_type=abstract

Binaries - Key to Comprehension of the Universe. Proceedings of a conference held June 8-12, 2009 in Brno, Czech Republic. Edite

Astronomy and Astrophysics

Astronomy

Scientific paper

High-precision and continuous satellite photometry of the MOST satellite (Microvariability and Oscillations of STars) lead to the detection of 16 new eclipsing binaries. Part of them have photometric amplitudes smaller than 0.1 mag and at the same time orbital periods longer than 10 days making them virtually inaccessible by the ground-based observations. Several known eclipsing binaries were also observed with unprecedented photometric precision leading to the determination of precise geometric elements and to detection of low-amplitude pulsations possibly caused by dynamical tides.

Affiliated with

Also associated with

No associations

Rating

MOST Satellite Photometry of Eclipsing Binaries 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 MOST Satellite Photometry of Eclipsing Binaries, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and MOST Satellite Photometry of Eclipsing Binaries will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1384917