Observations of Low Degree P-Modes with Odd L+M

Bibcode
1993ASPC...42..189P
Palle, P. L.; Perez-Hernandez, F.; Regulo, C.; Roca-Cortes, T.
Bibliographical reference

GONG 1992. Seismic Investigation of the Sun and Stars. Proceedings of a Conference held in Boulder, Colorado, August 11-14, 1993. Editor, Timothy M. Brown; Publisher, Astronomical Society of the Pacific #42, 1993.ISBN # 0-937707-61-9. LC # QB539.O83 G66 1992, P. 189, 1993

Advertised on:
1
1993
Number of authors
4
IAC number of authors
0
Citations
1
Refereed citations
1
Description
Not Available
Type
Non-refereed

It may interest you

  • Non-refereed
    EST preliminary design, status and future steps
    The European Solar Telescope (EST) aims to significantly improve our capabilities to observe the solar chromosphere and understanding the solar chromosphere represents one of the most challenging tasks in solar physics. EST incorporates the most innovative technology, with a simple and efficient design, and the most advanced instrumentation to
    Barreto, Mary et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..695B
    Citations
    0
  • Non-refereed
    The Galactic underdogs: characterizing a population of metal-poor stars with disc kinematics in the Milky Way
    To deepen our knowledge of the early history of the Milky Way, it is of particular interest to investigate the orbital and chemical properties of the most metal-poor stars, which are commonly associated with the oldest stars in our Universe. With the advent of astrometric (Gaia), spectroscopic (APOGEE, GALAH, LAMOST, Gaia-RVS), and photometric
    Gonzalez Rivera, Isaure et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..624G
    Citations
    0
  • Non-refereed
    Inferring stellar population properties from HST+JWST photometry using Normalizing Flows
    Spectral energy distributions (SEDs) encode information about the stellar populations within galaxies. By investigating the properties of these stars, such as their ages, masses, and metallicities, we can gain insights into the underlying physical processes that drive the growth and transformation of galaxies over cosmic time. For this purpose, we
    Iglesias Navarro, Patricia et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..225I
    Citations
    0