V1187 Herculis: A Red Novae progenitor, and the most extreme mass ratio binary known

Ronald G. Samec; Heather Chamberlain; Daniel Caton; Russell Robb; Danny R. Faulkner

doi:10.1017/S1743921319002485

V1187 Herculis: A Red Novae progenitor, and the most extreme mass ratio binary known

Ronald G. Samec
, Heather Chamberlain
, Daniel Caton
, Russell Robb
, Danny R. Faulkner

Appalachian State University

Pisgah Astronomical Research Institute
University of Victoria
Johnson Observatory

Research output: Contribution to journal › Article › peer-review

Original language	English
Pages (from-to)	288-293
Number of pages	6
Journal	Proceedings of the International Astronomical Union
Volume	14
DOIs	https://doi.org/10.1017/S1743921319002485
State	Published - Aug 1 2018

ASJC Scopus Subject Areas

Astronomy and Astrophysics
Space and Planetary Science

Keywords

stars: individual: V1187 Her
Stars:binaries: eclipsing

Access to Document

10.1017/S1743921319002485

Cite this

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title = "V1187 Herculis: A Red Novae progenitor, and the most extreme mass ratio binary known",

keywords = "stars: individual: V1187 Her, Stars:binaries: eclipsing",

author = "Samec, \{Ronald G.\} and Heather Chamberlain and Daniel Caton and Russell Robb and Faulkner, \{Danny R.\}",

note = "Publisher Copyright: {\textcopyright} International Astronomical Union 2019.",

year = "2018",

month = aug,

day = "1",

doi = "10.1017/S1743921319002485",

language = "English",

volume = "14",

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journal = "Proceedings of the International Astronomical Union",

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T2 - A Red Novae progenitor, and the most extreme mass ratio binary known

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AU - Chamberlain, Heather

AU - Caton, Daniel

AU - Robb, Russell

AU - Faulkner, Danny R.

PY - 2018/8/1

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KW - stars: individual: V1187 Her

KW - Stars:binaries: eclipsing

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SP - 288

EP - 293

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

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