Stellar Distribution in the Galactic Disk from NIR Color-Magnitude Diagrams

Bibcode
2004ASSL..315..221C
DOI
10.1007/1-4020-2620-X_44
Cabrera-Lavers, A.; Garzón, F.; Hammersley, P.
Bibliographical reference

How Does the Galaxy Work? A Galactic Tertulia with Don Cox and Ron Reynolds. Edited by Emilio J. Alfaro, Instituto de Astrofica de Andalucía (CSIC), Granada, Spain; Enrique Pérez, Instituto de Astrofíxica de Andalucía (CSIC), Granada, Spain; José Franco, Instituto de Astronomía, UNAM, México. ASTROPHYSICS AND SPACE SCIENCE LIBRARY Volume 315. ISBN 1-4020-2619-6 (HB); ISBN 1-4020-2620-X (e-book). Published by Kluwer Academic Publishers, Dordrecht, The Netherlands, 2004, p.221

Advertised on:
10
2004
Number of authors
3
IAC number of authors
3
Citations
0
Refereed citations
0
Description
We analyze the stellar distribution in the Galactic disk via NIR color-magnitude diagrams (CMDs). Extinction measurements in the K band are also extracted from the diagrams both for supporting stellar counts predictions of the Besaçon and "SKY" models and for comparing with a three dimensional model of the Galactic extinction. The method is based on extracting a well known stellar population from the CMDs providing a simple empirical way to obtain the stellar density and interstellar extinction along a line of sight.
Type
Non-refereed

It may interest you

  • Non-refereed
    Study of basaltic asteroids through their phase curves
    Introduction Classified as type-V, the basaltic asteroids of the Main Belt (MB), for the most part, are connected to Vesta's dynamic family. However, since the discovery of the V-type asteroid (1459) Magnya in the outer MB, several new asteroids have been found in different regions, including V-types from inner regions not belonging to the Vesta
    Arcoverde, Plicida et al.

    Advertised on:

    9
    2024
    Bibcode
    2024EPSC...17..999A
    Citations
    0
  • Non-refereed
    NIRPS near-infrared spectrograph: AITV phase at ESO3.6m/La Silla
    NIRPS is a fiber-fed AO nIR spectrograph working simultaneously with HARPS at the La Silla-ESO 3.6m telescope. The cryogenic spectrograph operating at 75K employs a cross-dispersed echelle grating (R4), covering a wavelength range of 0.98-1.80 microns in a single image using a Teledyne Hawaii-4RG infrared detector. In early 2022, the NIRPS
    Malo, Lison et al.

    Advertised on:

    7
    2024
    Bibcode
    2024SPIE13096E..46M
    Citations
    0
  • Non-refereed
    Transport, handling, and integration of the adaptive optics system for GTC: from the laboratory to the telescope
    The Gran Telescopio de Canarias Adaptive Optics System (GTCAO) is currently in its commissioning phase at Roque de Los Muchachos Observatory (ORM). The GTCAO is a single-conjugated post-focal system equipped with a Shack- Hartmann Wavefront Sensor (WFS) and a Deformable Mirror (DM) conjugated to the pupil, achieving a Strehl Ratio of 65% in the K
    González Carretero, Eduardo D. et al.

    Advertised on:

    7
    2024
    Bibcode
    2024SPIE13096E..96G
    Citations
    0