Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apjs..107..739h&link_type=abstract
Astrophysical Journal Supplement v.107, p.739
Astronomy and Astrophysics
Astronomy
4
Galaxies: Ism, Galaxies: Individual Ngc Number: Ngc 4670, Galaxies: Nuclei, Radio Lines: Galaxies
Scientific paper
We present a moderate resolution H I map of the amorphous galaxy NGC 4670. Our previous lower resolution data had shown a symmetric H I distribution centered on the single supergiant H II region and highly concentrated to the center of the galaxy. We now resolve the central H I distribution into three clouds, with the eastern cloud located on the central H II region and 1.1 kpc from the westernmost cloud. Masses of the clouds are of order 108 Msun and are associated with the intense central star formation that has produced a luminous, compact star cluster. The central gas surface density is very high at the new resolution, and the surface density drops off rapidly with radius. We determine a rotation curve for the galaxy; however, the low and uncertain value of the inclination (i ˜28°) and the possible presence of a warp make the derived rotation speed (VR ˜110 km s-1) quite uncertain. There is some correspondence between features in the H I distribution and locations of Hα loops and filaments that emanate from the central H II region.
Gallagher John S. III
Hunter Deidre Ann
van Woerden Hugo
No associations
LandOfFree
Neutral Hydrogen Observations of the Amorphous Galaxy NGC 4670 at Moderate Spatial Resolution does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Neutral Hydrogen Observations of the Amorphous Galaxy NGC 4670 at Moderate Spatial Resolution, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Neutral Hydrogen Observations of the Amorphous Galaxy NGC 4670 at Moderate Spatial Resolution will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-820036