Radial Velocity Measurements Based on FORS2 and FLAMES Spectra

Bibcode
2008eic..work...41M
DOI
10.1007/978-3-540-76963-7_5
Monelli, M.; Nonino, M.; Bono, G.; François, P.; Thévenin, F.; Buonanno, R.; Caputo, F.; Corsi, C. E.; Pulone, L.; Smith, H. A.; Stetson, P. B.; Walker, A. R.
Referencia bibliográfica

The 2007 ESO Instrument Calibration Workshop, ESO Astrophysics Symposia European Southern Observatory. ISBN 978-3-540-76962-0. Springer-Verlag Berlin Heidelberg, 2008, p. 41

Advertised on:
0
2008
Número de autores
12
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
We present an extensive spectroscopic investigation on evolved old- and intermediate-age stellar tracers of the Carina dSph galaxy. We discuss the approach we devised to calibrate the two multi-object spectrographs (FLAMES, FORS2) available at the European Southern Observatory. Pros and cons of the two instruments are also mentioned. Finally, we present preliminary results concerning the radial velocity measurements and the comparison with data from the literature
Tipo
Sin árbitro

Te puede interesar

  • Sin árbitro
    Constraining atmospheric evaporation timescales on young planets with systematic H and He transmission observations
    During the early stages of planetary formation, planets undergo strong changes in their physical and orbital properties due to internal and external forces, which also affect their primordial atmospheres composed mainly of H and He. The study of planets in these early stages and their comparison with the more mature planet population is crucial for
    Orell-Miquel, Jaume et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf.1494O
    Número de citas
    0
  • Sin árbitro
    Bar pattern speeds across the Hubble Sequence
    Bars are ellipsoidal-like structures that appears in the inner regions of a large fraction of discs of galaxies. Bars universal features present at all galactic masses, morphological types and across the Hubble time. Stars forming bars follow elongated orbits aligned with the bar major-axis. These barred structures rotate as a coherent structure
    Aguerri, J. Alfonso L.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf.2582A
    Número de citas
    0
  • Sin árbitro
    Confronting Dark Matter Models with Nearby Dwarf Irregular Galaxies
    Dwarf irregular galaxies, due to their lower masses, relative isolation, and high-quality data availability, are ideal laboratories to test various models of dark matter. In particular, the existence, morphology and formation of central cores in dwarf galaxies has been a contentious issue in the literature in light of apparent tensions with the
    Bañares Hernández, Andrés et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf.1858B
    Número de citas
    0