Explore
Theory and Observation of Active B-type Stars
0 Ungluers have
Faved this Work
Login to Fave
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 B-type stars seen on various time and spatial scales is often connected to the formation and dissipation of these disks. Although the possible roles of radiation, rotation, pulsation, and binarity in pulling material off the stars have been explored in detail in the past few decades, the relevant physical processes involved in the formation of sustainable disks and their dynamical evolution are still unclear and a matter of debate.This Special Issue intends to provide a comprehensive update on the state of knowledge in the field of active B-type stars. It combines reviews and selected contributions on recent groundbreaking advancements in the comprehension of these peculiar objects from both a theoretical and an observational perspective. These new insights form the basis for exploring complex physical phenomena to verify the different scenarios proposed for the evolution and variability of stars and their circumstellar environment of the diverse classes of active B-type stars.
This book is included in DOAB.
Why read this book? Have your say.
You must be logged in to comment.
Rights Information
Are you the author or publisher of this work? If so, you can claim it as yours by registering as an Unglue.it rights holder.Downloads
This work has been downloaded 14 times via unglue.it ebook links.
- 14 - pdf (CC BY) at Unglue.it.
Keywords
- (stars:) circumstellar matter
- analytical methods
- Archive
- Astronomy, space & time
- Be
- Be circumstellar matter
- Be stars
- binaries: eclipsing
- binaries: general
- circumstellar disks
- circumstellar matter
- circumstellar matter: jets and outflows
- early-type emission stars
- early-type stars
- early-type variable stars
- emission line
- Gaia
- galaxies: individual
- HD 36030
- Hydrodynamics
- mass-loss stars
- massive stars
- Mathematics & science
- methods: statistical methods: numerical
- NGC 247
- NGC 253
- NGC 300
- NGC 3109
- NGC 55
- NGC 7793
- Numerical methods
- open star clusters
- outflows
- Physics
- Reference, information & interdisciplinary subjects
- Research & information: general
- S Doradus infrared
- star evolution
- star variables
- stars activity
- stars binaries spectroscopic
- stars flares
- stars individual
- Stars: activity
- Stars: chemically peculiar
- stars: early-type
- stars: emission-line
- stars: emission-line, Be
- Stars: evolution
- stars: individual Z CMa
- stars: individual: MWC 645
- stars: individual: MX Pup, π Aqr
- stars: infrared
- Stars: magnetic field
- stars: mass-loss
- stars: massive
- stars: oscillations (including pulsations)
- stars: peculiar
- stars: peculiar (except chemically peculiar)
- Stars: rotation
- stars: supergiants
- stars: symbiotic, binaries
- stars: winds
- supergiant stars
- Techniques: spectrophotometric
- techniques: spectroscopic
- WLM
Links
DOI: 10.3390/books978-3-0365-9122-3Editions