Winds Driven by Super-Star Clusters

Bibcode
2004RMxAC..22..152S
Silich, S.; Tenorio-Tagle, G.; Rodríguez-González, A.; Muñoz-Tuñon, C.
Referencia bibliográfica

Gravitational Collapse: From Massive Stars to Planets. / First Astrophysics meeting of the Observatorio Astronomico Nacional. / A meeting to celebrate Peter Bodenheimer for his outstanding contributions to Astrophysics. (Eds. G. García-Segura, G. Tenorio-Tagle, J. Franco, & H. W. Yorke) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 22, pp. 152-155 (2004) (http://www.astroscu.unam.mx/~rmaa/)

Fecha de publicación:
12
2004
Número de autores
4
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
Here we present a self-consistent stationary solution for spherically symmetric winds driven by massive star clusters under the impact of radiative cooling. We demonstrate that cooling may modify drastically the distribution of temperature if the rate of injected energy approaches a critical value and that the stationary wind solution does not exist if the energy deposition rate exceeds this limit. Finally, we discuss the expected appearance of the supergalactic winds driven by multiple super-star clusters.
Tipo
Sin árbitro
Galaxias
Cúmulos de estrellas

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