Panel discussion I

F. Allard, A. Batten, E. Budding, E. Devinney, P. Eggleton, A. Hatzes, I. Hubeny, W. Kley, H. Lammer, A. Linnell, V. Trimble, R. E. Wilson

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

Abstract

M. Richards: Several talks today have expressed fuzzy boundaries to describe the objects called stars. Is the following classification correct? Are stars restricted to objects that have masses greater than 0.089 solar masses and begin making energy with hydrogen burning? Do we include the stellar remnants: the white dwarfs and neturon stars? Do we include the brown dwarfs because they burn lithium or deuterium. We know that planets are not in this group since they have no energy production.

Original languageEnglish (US)
Title of host publicationFrom Interacting Binaries to Exoplanets
Subtitle of host publicationEssential Modeling Tools
EditorsMercedes Richards, Ivan Hubeny
Pages145-152
Number of pages8
EditionS282
DOIs
StatePublished - Jul 1 2011

Publication series

NameProceedings of the International Astronomical Union
NumberS282
Volume7
ISSN (Print)1743-9213
ISSN (Electronic)1743-9221

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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    Allard, F., Batten, A., Budding, E., Devinney, E., Eggleton, P., Hatzes, A., Hubeny, I., Kley, W., Lammer, H., Linnell, A., Trimble, V., & Wilson, R. E. (2011). Panel discussion I. In M. Richards, & I. Hubeny (Eds.), From Interacting Binaries to Exoplanets: Essential Modeling Tools (S282 ed., pp. 145-152). (Proceedings of the International Astronomical Union; Vol. 7, No. S282). https://doi.org/10.1017/S1743921311027244