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Theory and Observation of Active B-type Stars

Active B-type stars are defined by their characteristic emission formed in a dense environment. Among them are the classical Be stars, which are surrounded by ionized gaseous disks, and B[e] stars, whose disks are so dense that even molecules and dust can form within them. The variability of active...

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Salvato in:
Natura: Online
Lingua:inglese
Pubblicazione: MDPI - Multidisciplinary Digital Publishing Institute 2023
Soggetti:
stars: individual: α Eri, α Col, ω Car, η Cen
archive
stars: emission-line, Be
stars: early-type
(stars:) circumstellar matter
stars: peculiar (except chemically peculiar)
Be stars
early-type emission stars
circumstellar disks
early-type variable stars
open star clusters
Gaia
Techniques: spectrophotometric
Stars: activity
Stars: emission-line, B, Bn, Be, B[e], Bm
Stars: rotation
Stars: evolution
Stars: chemically peculiar
Stars: magnetic field
stars flares
stars activity
stars binaries spectroscopic
early-type stars
stars individual
HD 36030
circumstellar matter: jets and outflows
stars: individual Z CMa
stars: emission-line
Be
stars: massive
stars: mass-loss
hydrodynamics
analytical methods
numerical methods
methods: statistical methods: numerical
binaries: eclipsing
stars: oscillations (including pulsations)
stars: peculiar
stars: individual: MWC 645
circumstellar matter
binaries: general
techniques: spectroscopic
stars: supergiants
stars: winds
outflows
massive stars
mass-loss stars
star evolution
emission line
Be circumstellar matter
supergiant stars
star variables
S Doradus infrared
galaxies: individual
WLM
NGC 55
NGC 247
NGC 253
NGC 300
NGC 3109
NGC 7793
stars: symbiotic, binaries
stars: infrared
stars: individual: MX Pup, π Aqr
thema EDItEUR::G Reference, Information and Interdisciplinary subjects::GP Research and information: general
thema EDItEUR::P Mathematics and Science::PH Physics
thema EDItEUR::P Mathematics and Science::PG Astronomy, space and time
Accesso online:ONIX_20231130_9783036591230_301
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