Star formation enhancement characteristics in interacting galaxies

Bibcode
2015IAUS..309..354Z
DOI
10.1017/S174392131401045X
Zaragoza-Cardiel, J.; Beckman, J. E.; Font, J.; Camps-Fariña, A.; García-Lorenzo, B.; Erroz-Ferrer, S.
Referencia bibliográfica

Galaxies in 3D across the Universe, Proceedings of the International Astronomical Union, IAU Symposium, Volume 309, pp. 354-354

Fecha de publicación:
2
2015
Número de autores
6
Número de autores del IAC
6
Número de citas
0
Número de citas referidas
0
Descripción
We have observed 12 interacting galaxies using the Fabry-Perot interferometer GHαFaS (Galaxy Hα Fabry-Perot system) on the 4.2m William Herschel Telescope (La Palma). We have extracted the physical properties (sizes, Hα luminosity and velocity dispersion) of 236 HII regions for the full sample of interacting galaxies. We have derived the physical properties of 664 HII regions for a sample of 28 isolated galaxies observed with the same instrument in order to compare both populations of HII regions, finding that there are brighter and denser star forming regions in the interacting galaxies compared with the isolated galaxies sample.
Tipo
Sin árbitro
Galaxias

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