Theory and Observation of Active B-type Stars

• Outros Autores: Cidale, Lydia Sonia (Editor), Kraus, Michaela (Editor), Arias, María Laura (Editor)
• Formato: Recurso Electrónico Capítulo de Livro
• Idioma: inglês
• Publicado em: Basel MDPI - Multidisciplinary Digital Publishing Institute 2023
• Assuntos: Research & information: general; Physics; Astronomy, space & time; 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
• Acesso em linha: DOAB: download the publication; DOAB: description of the publication

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...