The Liège Oscillation code

Bibcode
2008Ap&SS.316..149S
DOI
10.1007/s10509-007-9577-6
Scuflaire, R.; Montalbán, J.; Théado, S.; Bourge, P.-O.; Miglio, A.; Godart, M.; Thoul, A.; Noels, A.
Bibliographical reference

Astrophysics and Space Science, Volume 316, Issue 1-4, pp. 149-154

Advertised on:
8
2008
Journal
Astrophysics and Space Science
Number of authors
8
IAC number of authors
0
Citations
121
Refereed citations
109
Description
The Liège Oscillation code can be used as a stand-alone program or as a library of subroutines that the user calls from a Fortran main program of his own to compute radial and nonradial adiabatic oscillations of stellar models. We describe the variables and the equations used by the program and the methods used to solve them. A brief account is given of the use and the output of the program.
Type
Refereed

It may interest you

  • Refereed
    An ultra-short-period super-Earth with an extremely high density and an outer companion
    We present the discovery and characterization of a new multi-planetary system around the Sun-like star K2-360 (EPIC 201595106). K2-360 was first identified in K2 photometry as the host of an ultra-short-period (USP) planet candidate with a period of 0.88 d. We obtained follow-up transit photometry, confirming the star as the host of the signal
    Livingston, John H. et al.

    Advertised on:

    11
    2024
    Bibcode
    2024NatSR..1427219L
    Citations
    0
  • Refereed
    High-resolution observations of recurrent jets from an arch filament system
    Context. Solar jets are collimated plasma ejections along magnetic field lines observed in hot (extreme-ultraviolet (EUV) jets) and cool (chromospheric surges) temperature diagnostics. Their trigger mechanisms and the relationship between hot and cool jets are still not completely understood. Aims. We aim to investigate the generation of a sequence
    Joshi, Reetika et al.

    Advertised on:

    11
    2024
    Bibcode
    2024A&A...691A.198J
    Citations
    0
  • Refereed
    KISS: Instrument Description and Performance
    Kinetic inductance detectors (KIDs) have been proven as reliable systems for astrophysical observations, especially in the millimeter range. Their compact size enables them to optimally fill the focal plane, thus boosting sensitivity. The KIDs Interferometric Spectral Surveyor (KISS) instrument is a millimeter camera that consists of two KID arrays
    Macías-Pérez, J. F. et al.

    Advertised on:

    11
    2024
    Bibcode
    2024PASP..136k4505M
    Citations
    0