What happens when a hot star shines on a cool one?

Katrina Exter, Travis Barman, Don Pollacco, Vladislav Pustynski, Steve Bell, Izold Pustylnik

Research output: Chapter in Book/Report/Conference proceedingConference contribution

1 Scopus citations

Abstract

In this, we discuss our on-going work observing the effects, and modeling the physical processes, of the irradiation of a cool star by its hot companion in close-binary systems. In particular, we present here some data and results on the post common-envelope systems EC 11575-1845 and UU Sge.

Original languageEnglish (US)
Title of host publicationINTERACTING BINARIES
Subtitle of host publicationAccretion, Evolution, and Outcomes
Pages561-564
Number of pages4
DOIs
StatePublished - May 21 2005
EventINTERACTING BINARIES: Accretion, Evolution, and Outcomes - Cefalu, Sicily, Italy
Duration: Jul 4 2004Jul 10 2004

Publication series

NameAIP Conference Proceedings
Volume797
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Other

OtherINTERACTING BINARIES: Accretion, Evolution, and Outcomes
CountryItaly
CityCefalu, Sicily
Period7/4/047/10/04

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Keywords

  • Close binary stars
  • Irradiation (modeling, observations)

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Exter, K., Barman, T., Pollacco, D., Pustynski, V., Bell, S., & Pustylnik, I. (2005). What happens when a hot star shines on a cool one? In INTERACTING BINARIES: Accretion, Evolution, and Outcomes (pp. 561-564). (AIP Conference Proceedings; Vol. 797). https://doi.org/10.1063/1.2130285