BVRCIC Observations, Analysis, and Spectra of The Most Extreme Mass Ratio (Totally Eclipsing) W UMa Binary, V1187 Herculis-Reference-Cited by-同舟云学术

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BVRCIC Observations, Analysis, and Spectra of The Most Extreme Mass Ratio (Totally Eclipsing) W UMa Binary, V1187 Herculis

Published:2019-03-26 Issue:999 Volume:131 Page:054203
ISSN:0004-6280
Container-title:Publications of the Astronomical Society of the Pacific
language:
Short-container-title:PASP

Author:

Caton Daniel,Gentry Davis R.,Samec Ronald G.,Chamberlain Heather,Robb Russell,Faulkner Danny R.,Hill Robert

Publisher

IOP Publishing

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/1538-3873/131/i=999/a=054203/pdf

Reference34 articles.

1. ROTSE All-Sky Surveys for Variable Stars. I. Test Fields

2. The minimum mass ratio of W UMa-type binary systems

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1. The first CCD photometric studies of the member eclipsing binary ZTFJ015003.88+534734.1 in the newly discovered young open cluster UBC 188;New Astronomy;2024-08

2. The critical mass ratio for W UMa-type contact binary systems;Serbian Astronomical Journal;2024

3. Improved Period Variations of 32 Contact Binaries with Rapidly Decreasing Periods in the Galactic Bulge;The Astronomical Journal;2023-12-13

4. Flares confirmed for the first time to be from the primary component of an eclipsing binary;Monthly Notices of the Royal Astronomical Society;2023-10-25

5. First investigations of 14 neglected, late-type contact binaries;Astrophysics and Space Science;2023-09

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