Disk-loss and disk-renewal phases in classical be stars. II. Contrasting with stable and variable disks

From National Research Council Canada

DOIResolve DOI: https://doi.org/10.1088/0004-637X/786/2/120
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Affiliation
  1. National Research Council of Canada. National Science Infrastructure
FormatText, Article
Subjectcircumstellar matter; stars: individual (pi Aquarii, 60 Cygni, 48 Librae, psi Persei, phi Persei, 28 Cygni, 66 Ophiuchi, gamma Casseopia, omega Orionis, FY CMa, 59 Cyg)
Abstract
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PublisherAmerican Astronomical Society
IOP Publishing
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LanguageEnglish
Peer reviewedYes
NPARC number21272656
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Record identifier65701775-4d89-48e2-9a4b-3875b9a2ca60
Record created2014-12-03
Record modified2020-04-22
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