Far IR Properties of AGNs. The AGN-Starburst Connection

Bibcode
2005AIPC..761..437M
DOI
10.1063/1.1913962
Masegosa, J.; Márquez, I.; Dultzin-Hacyan, D.; González-Martín, O.
Referencia bibliográfica

THE SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data; International Workshop. AIP Conference Proceedings, Volume 761, pp. 437-440 (2005).

Fecha de publicación:
4
2005
Número de autores
4
Número de autores del IAC
0
Número de citas
1
Número de citas referidas
1
Descripción
With the main goal of investigating the AGN and/or Starburst nature of LINERs, we have studied their FIR properties. Based on the classical indicators of Star Formation activity S25/S100 and the S60/S100 ratios, we have confirmed their heterogeous nature and they can be separated in three groups: normal spiral galaxies with low level nuclear star formation, galaxies with enhanced star formation to be bonafide candidates to Starburst systems, and ongoing mergers with very peculiar SPR up to a few hundreds.
Tipo
Sin árbitro
Galaxias espirales

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