THE STELLAR POPULATION OF h AND χ PERSEI: CLUSTER PROPERTIES, MEMBERSHIP, AND THE INTRINSIC COLORS AND TEMPERATURES OF STARS-Reference-Cited by-同舟云学术

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THE STELLAR POPULATION OF h AND χ PERSEI: CLUSTER PROPERTIES, MEMBERSHIP, AND THE INTRINSIC COLORS AND TEMPERATURES OF STARS

Published:2010-01-14 Issue:2 Volume:186 Page:191-221
ISSN:0067-0049
Container-title:The Astrophysical Journal Supplement Series
language:
Short-container-title:ApJS

Author:

Currie Thayne,Hernandez Jesus,Irwin Jonathan,Kenyon Scott J.,Tokarz Susan,Balog Zoltan,Bragg Ann,Berlind Perry,Calkins Mike

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference96 articles.

1. The Monitor project: searching for occultations in young open clusters

2. TiO and H2O Absorption Lines in Cool Stellar Atmospheres

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