SIMBAD references

2004AJ....127..736H - Astron. J., 127, 736-757 (2004/February-0)

A study of the distribution of star-forming regions in luminous infrared galaxies by means of Hα imaging observations.

HATTORI T., YOSHIDA M., OHTANI H., SUGAI H., ISHIGAKI T., SASAKI M., HAYASHI T., OZAKI S., ISHII M. and KAWAI A.

Abstract (from CDS):

We performed Hα imaging observations of 22 luminous infrared galaxies to investigate how the distribution of star-forming regions in these galaxies is related to galaxy interactions. Based on correlation diagrams between Hα flux and continuum emission for individual galaxies, a sequence for the distribution of star-forming regions was found: very compact (∼100 pc) nuclear starbursts with almost no star-forming activity in the outer regions (type 1), dominant nuclear starbursts ≲1 kpc in size with a negligible contribution from the outer regions (type 2), nuclear starbursts ≳1 kpc in size with a significant contribution from the outer regions (type 3), and extended starbursts with relatively faint nuclei (type 4). These classes of star-forming regions were found to be strongly related to global star-forming properties, such as star formation efficiency, far-infrared color, and dust extinction. There was a clear tendency for the objects with more compact distributions of star-forming regions to show a higher star formation efficiency and hotter far-infrared color. An appreciable fraction of the sample objects were dominated by extended starbursts (type 4), which is unexpected in the standard scenario of interaction-induced starburst galaxies. We also found that the distribution of star-forming regions was weakly but clearly related to galaxy morphology: severely disturbed objects had a more concentrated distribution of star-forming regions. This suggests that the properties of galaxy interactions, such as dynamical phase and orbital parameters, play a more important role than the internal properties of progenitor galaxies, such as dynamical structure or gas mass fraction. We also discuss the evolution of the distribution of star-forming regions in interacting galaxies.

Abstract Copyright:

Journal keyword(s): Galaxies: Interactions - Galaxies: Starburst

Simbad objects: 36

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2004AJ....127..736H and select 'bookmark this link' or equivalent in the popup menu


2021.06.24-09:24:51

© Université de Strasbourg/CNRS

    • Contact