The extended gaseous and dark components of M33

Details The extended gaseous and dark components of M33 The extended gaseous and dark components of M33

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000immm.proc...11c&link_type=abstract

The interstellar medium in M31 and M33. Proceedings 232. WE-Heraeus Seminar, 22-25 May 2000, Bad Honnef, Germany. Edited by El

Physics

Scientific paper

High sensitivity observations of the extended HI disk of M33 have given us a clue on many distinct properties of this nearby galaxy, such as the radial sharp cutoff of the HI surface density due to the UV ionizing flux, the warp of the outer disk, the rotation curve and the dark matter distribution out to 13 disk scalelengths. Results of recent observations of the molecular gas in this galaxy will also be briefly summarized.

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