Position-Velocity Diagrams in the Inner Regions of Disk Galaxies

Bibcode
2001ASPC..230..277F
Funes, J. G.; Pizzella, A.; Corsini, E. M.; Cappellari, M.; Scarlata, M. C.; Bertola, F.; Vega Beltrán, J. C.
Bibliographical reference

in Galaxy Disks and Disk Galaxies, proceeding of a conference held in Rome, Italy, June 12-16, 2000 at the Pontifical Gregorian University and sponsored by the Vatican Observatory. ASP Conference Series, Vol. 230. Edited by José G. Funes, S. J. and Enrico Maria Corsini. San Francisco: Astronomical Society of the Pacific. ISBN: 1-58381-063-3, 2001, pp. 277-278

Advertised on:
0
2001
Number of authors
7
IAC number of authors
1
Citations
0
Refereed citations
0
Description
Not Available
Type
Non-refereed

It may interest you

  • Non-refereed
    Accretion-induced variability of interacting red giant binaries masquerading as oscillations
    Symbiotic stars are strongly interacting binaries with long orbital periods, containing an evolved red giant and a white dwarf or a neutron star embedded in a circumbinary nebula. They constitute unique astrophysical laboratories important for understanding the binary evolution and diverse processes occurring also in many other types of
    Merc, Jaroslav et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..966M
    Citations
    0
  • Non-refereed
    2 Young 2 Furious - Challenges and opportunities in the study of young exoplanets
    Current theories of planetary evolution predict that infant giant planets have large radii and very low densities before they slowly contract to reach their final size after about several hundred million years. These theoretical expectations have remained untested for a long time, as the detection and characterization of very young planets is
    Suárez Mascareño, Alejandro

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf.2518S
    Citations
    0
  • Non-refereed
    The mysterious globular cluster population of NGC5846-UDG1 (MATLAS-2019)
    The number of globular clusters plays a fundamental role in understanding the early stages of galaxy formation. We know that the GC population of normal galaxies correlates with the amount of dark matter in these objects. Extending this analysis to the number of globulars in very low surface brightness galaxies is therefore key to understanding the
    Guerra Arencibia, Sergio et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..619G
    Citations
    0