Evidences for high-velocity superwinds in starburst galaxies from ISO spectroscopy

Details Evidences for high-velocity superwinds in starburst galaxies from ISO spectroscopy Evidences for high-velocity superwinds in starburst galaxies from ISO spectroscopy

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000newar..44..269c&link_type=abstract

New Astronomy Reviews, Volume 44, Issue 4-6, p. 269-273.

Astronomy and Astrophysics

Astronomy

Scientific paper

Using a composite model which consistently accounts for the coupled effect of shocks and photoionization by hot stars, we show that high-velocity (~400-600 kms-1) shocks in dense (~500-800 cm-3) clouds are necessary to reproduce some critical infrared line ratios observed by ISO in some typical nearby Starburst Nucleus Galaxies. These results are in good agreement with the powerful starburst-driven superwinds and highly pressured interstellar medium observed in these starburst galaxies.

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