Binary stars: selected topics on observations and physical processes

Bibcode
2001LNP...563.....L
Lázaro, C.; Arévalo, M. J.
Referencia bibliográfica

Binary stars: selected topics on observations and physical processes. Lectures held at the Astrophysics School XII organized by the European Astrophysics Doctoral Network (EADN) in La Laguna, Tenerife, Spain, 6 - 17 September 1999, Eds.: F. C. Lázaro, M. J. Arévalo, Lecture notes in physics, Vol.563. Physics and astronomy online library. Berlin: Springer, ISBN 3-540-41256-5, 2001, 327 pp.

Fecha de publicación:
2001
Número de autores
2
Número de autores del IAC
2
Número de citas
0
Número de citas referidas
0
Descripción
More than half of all stars in the Galaxy formed and evolved as binary systems and their study is essential for understanding stellar and galactic evolution. Six lectures in this book give both a readable introduction and an up-to-date review of nearly all aspects of current research into binary stars, including the range from common binaries to more exotic systems composed of white dwarfs, neutron stars and black holes.
Tipo
Sin árbitro

Te puede interesar

  • Sin árbitro
    A Systematic Search for and Characterization of White Dwarf Binaries Across the H-R Diagram
    White dwarfs (WDs) are the endpoint of evolution for 97% of stars. Most of these stars are in multiple systems, and a significant fraction of those are compact enough to exchange mass, altering the structures and subsequent evolution of both stars. The physical mechanisms that facilitate these mass exchanges include common envelope evolution, Roche
    Anguiano, Borja et al.

    Fecha de publicación:

    6
    2024
    Bibcode
    2024AAS...24410807A
    Número de citas
    0
  • Sin árbitro
    ROSALIA: ROman Sky Analyst for Low surface brightness Imaging & Astronomy
    Diffuse emission in the outskirts of galaxies, such as stellar tidal streams, galaxy stellar halos and intracluster light, provides important constraints on the structure and evolution of the Universe. However, such low surface brightness diffuse emission can be up to thousands of times dimmer (>29 AB mag/[square arcseconds]) than the sky
    Laine, Seppo et al.

    Fecha de publicación:

    6
    2024
    Bibcode
    2024AAS...24412902L
    Número de citas
    0
  • Sin árbitro
    The molecular gas perspective on the growth and death of H emitters in the Spiderweb protocluster at Alpha z=2.16
    Galaxy clusters at low redshift are dominated by massive quiescent galaxies hosting stellar populations 10 Gyrs old, indicating that they were formed in the early universe when clusters were still in the process of being assembled (i.e., protoclusters). The rapid growth of galaxies within protoclusters is driven by the efficient transformation of
    Martinez, J. M. P.

    Fecha de publicación:

    3
    2024
    Bibcode
    2024aecc.conf...12M
    Número de citas
    0