Star formation in stellar systems

Bibcode
1992sfss.conf.....T
Tenorio-Tagle, G.; Prieto, M.; Sanchez, F.
Referencia bibliográfica

Star Formation in Stellar Systems, Proceedings of the III Canary Islands Winter School of Astrophysics. Edited by G. Tenorio-Tagle, M. Prieto, and F. Sanchez. Cambridge: University of Cambridge Press, 1992.

Fecha de publicación:
1
1992
Número de autores
3
Número de autores del IAC
0
Número de citas
5
Número de citas referidas
2
Descripción
The present volume on stellar formation discusses basic physical principles relevant to such processes, regions of recent star formation, galaxy formation and evolution, and the history of star formation in galaxies. Also discussed are OB associations and superassociations, triggered star formations, violent star formation in merging galaxies, and large-scale propagating stellar formation.
Tipo
Sin árbitro
Formación estelar
Física estelar
Estrellas OB
Estrellas B
Galaxias en interacción
Galaxias con estallidos
Protostars
Estrellas binarias
Campos magnéticos interestelares
Via Láctea
Regiones H II
Núcleos activos de galaxias

Te puede interesar

  • Sin árbitro
    Performance of the image persistence model for Euclid infrared detectors
    Large-format infrared detectors are at the heart of major ground and space-based astronomical instruments, and the HgCdTe HxRG is the most widely used. The Near Infrared Spectrometer and Photometer (NISP) of the ESA's Euclid mission launched in July 2023 hosts 16 H2RG detectors in the focal plane. Their performance relies heavily on the effect of
    Kubik, B. et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13103E..15K
    Número de citas
    0
  • Sin árbitro
    HARMONI at ELT: athermal toroidal mirror mount for HARMONI pre-optics
    HARMONI is the high angular resolution optical and near-IR integral field spectrograph for the Extremely Large telescope (ELT). It covers a large spectral range from 470nm to 2450nm with resolving powers from 3300 to 18000 and spatial sampling from 60mas to 4mas. The Instrument Pre-Optics (IPO), a sub-system under the responsibility of the
    Hernández, Elvio et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13100E..34H
    Número de citas
    0
  • Sin árbitro
    HARMONI at ELT: project status and instrument overview
    HARMONI is the first light visible and near-IR integral field spectrograph for the ELT. It covers a large spectral range from 450 nm to 2450 nm with resolving powers from 3500 to 18000 and spatial sampling from 60 mas to 4 mas. It can operate in two Adaptive Optics modes - SCAO (including a High Contrast capability) and LTAO - or with NOAO. The
    Thatte, Niranjan A. et al.

    Fecha de publicación:

    7
    2024
    Bibcode
    2024SPIE13096E..14T
    Número de citas
    0