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

doi:10.1017/S1743921311027244

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 proceeding › Conference 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 language	English (US)
Title of host publication	From Interacting Binaries to Exoplanets
Subtitle of host publication	Essential Modeling Tools
Editors	Mercedes Richards, Ivan Hubeny
Pages	145-152
Number of pages	8
Edition	S282
DOIs	https://doi.org/10.1017/S1743921311027244
State	Published - Jul 2011
Externally published	Yes

Publication series

Name	Proceedings of the International Astronomical Union
Number	S282
Volume	7
ISSN (Print)	1743-9213
ISSN (Electronic)	1743-9221

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.1017/S1743921311027244

Cite this

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

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

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AU - Budding, E.

AU - Devinney, E.

AU - Eggleton, P.

AU - Hatzes, A.

AU - Hubeny, I.

AU - Kley, W.

AU - Lammer, H.

AU - Linnell, A.

AU - Trimble, V.

AU - Wilson, R. E.

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AB - 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.

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Panel discussion I

Abstract

Publication series

ASJC Scopus subject areas

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