Volume 399, Number 3, March I 2003
|Page(s)||833 - 855|
|Published online||14 February 2003|
ISOCAM view of the starburst galaxies M 82, NGC 253 and NGC 1808 *
CEA/DSM/DAPNIA/Service d'Astrophysique, CE Saclay, 91191 Gif-sur-Yvette Cedex, France
2 Astronomy Department, Cornell University, Ithaca, NY 14853, USA
3 Observatoire de Paris (Chercheur Associé.) , LERMA, 61 avenue de l'Observatoire, 75014 Paris, France
4 Max-Planck-Institute für extraterrestrische Physik, Postfach 1312, 85741 Garching, Germany
5 Instituto de Astronomía y Física del Espacio, cc 67, suc 28, 1428 Buenos Aires, Argentina
Corresponding author: N. M. Förster Schreiber, email@example.com
Accepted: 15 November 2002
We present results of mid-infrared – spectrophotometric imaging of the starburst galaxies M 82, NGC 253, and NGC 1808 from the ISOCAM instrument on board the Infrared Space Observatory . The mid-infrared spectra of the three galaxies are very similar in terms of features present. The continuum attributed to very small dust grains (VSGs) exhibits a large spread in intensity relative to the short-wavelength emission. We find that the 15m dust continuum flux density correlates well with the fine-structure  6.99m line flux and thus provides a good quantitative indicator of the level of star formation activity. By contrast, the – region dominated by emission from polycyclic aromatic hydrocarbons (PAHs) has a nearly invariant shape. Variations in the relative intensities of the PAH features are nevertheless observed, at the – level. We illustrate extinction effects on the shape of the mid-infrared spectrum of obscured starbursts, emphasizing the differences depending on the applicable extinction law and the consequences for the interpretation of PAH ratios and extinction estimates. The relative spatial distributions of the PAH, VSG, and  6.99m emission between the three galaxies exhibit remarkable differences. The size of the mid-infrared source is much smaller than the optical extent of our sample galaxies and – of the IRAS 12m flux is recovered within the ISOCAM field of view, indicating that the nuclear starburst dominates the total mid-infrared emission while diffuse light from quiescent disk star formation contributes little.
Key words: galaxies: individual: M 82, NGC 253, NGC 1808 / galaxies: ISM / galaxies: starburst / infrared: galaxies / infrared: ISM
© ESO, 2003
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.