UV variability of IRAS 13224-3809.

Bibcode
1994vsf..book..256M
Mas-Hesse, J. M.; Rodriguez-Pascual, P. M.; Sanz Fernandez de Cordoba, L.; Boller, T.
Bibliographical reference

"Violent Star Formation: From 30 Doradus to QSOs, Proceedings of the first IAC-RGO meeting held in

Advertised on:
0
1994
Number of authors
4
IAC number of authors
0
Citations
0
Refereed citations
0
Description
Not Available
Type
Non-refereed
Infrared galaxies

It may interest you

  • Non-refereed
    Application of Bayesian Inference to disentangle CMB foregrounds
    Both Galactic dust emission and Cosmic infrared background anisotropies (CIB) act as a dominant foreground contaminant for the measurements of the CMB anisotropies (intensity and polarization) at the frequency range above 217 GHz. The Galactic dust and CIB share a similar form of spectral energy distribution, which makes it harder to disentangle
    Adak, Debabrata et al.

    Advertised on:

    1
    2024
    Bibcode
    2024asi..confP..71A
    Citations
    0
  • Non-refereed
    Constraining stellar and orbital co-evolution through ensemble seismology of solar-like oscillators in binary systems
    The evolution of stars and their hosting binary systems is a highly interactive process and cannot be investigated in a segregated manner. Due to the constraints drawn by stellar binarity, oscillating red-giant stars in binary systems represent a unique opportunity to study the details of the structure and evolution of stars in the advanced phases
    Beck, P. G. et al.

    Advertised on:

    3
    2024
    Bibcode
    2024aecc.conf...24B
    Citations
    0
  • Non-refereed
    Triple-Double Radio Galaxies: Clues for understanding recurrent AGN activity
    Using LOFAR Two-metre Sky Survey (LoTSS), we discovered three cycles of episodic jet activity (J1225+4011, Chavan et al. 2023, MNRAS) in a giant radio galaxy, which is an extremely rare class of restarted Active Galactic Nuclei (AGN), making it only fourth of its kind. It is also called 'Triple-Double Radio Galaxy' (TDRG). J1225+4011 extends up to
    Chavan, Kshitij et al.

    Advertised on:

    1
    2024
    Bibcode
    2024asi..confP..64C
    Citations
    0