Bar Strengths in Galaxies as Measured from INGRID Images

Bibcode
2002INGN....6....3K
Knapen, J. H.; Block, D. L.; Buta, R.; Puerari, I.; Elmegreen, B. G.; Stedman, S.; Elmegreen, D. M.
Referencia bibliográfica

The Newsletter of the Isaac Newton Group of Telescopes (ING Newsl.), issue no. 6, p. 3-6.

Fecha de publicación:
10
2002
Número de autores
7
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
We describe results from our study of a sample of spiral galaxies of a wide range of Hubble types on the basis of near-IR imaging obtained with INGRID on the WHT. We focus on the determination of bar torques, or bar strengths, from our images, and show that this bar strength only very weakly correlates with de Vaucouleurs bar type, or with bar axis ratio.
Tipo
Sin árbitro
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