The distance to low-latitude negative-velocity clouds in the galactic anticenter

Details The distance to low-latitude negative-velocity clouds in the galactic anticenter The distance to low-latitude negative-velocity clouds in the galactic anticenter

Publishing date

Apr 1977

URL

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...213..379d&link_type=abstract

Journals

Astrophysical Journal, Part 1, vol. 213, Apr. 15, 1977, p. 379-385.

Science

Astronomy and Astrophysics

Field

Astrophysics

Additional info 2

12

Additional info 3

Galactic Structure, Hydrogen Clouds, Spiral Galaxies, Supernova Remnants, Astronomical Maps, Brightness Temperature, Interstellar Matter, Nebulae

Type

Scientific paper

Abstract

A complex of low-latitude negative-velocity clouds in the anticenter, which has been interpreted as a distant spiral arm and as tidal debris from a companion hydrogen galaxy, is shown to be local (not more than 2 kpc). The distance is based on an association between two hydrogen jets in this complex and the supernova remnants IC 443 and the Origem Loop. The implication of the relationship between the jets and the remnants is discussed.

Affiliated with

Also associated with

No associations

Rating

The distance to low-latitude negative-velocity clouds in the galactic anticenter 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 The distance to low-latitude negative-velocity clouds in the galactic anticenter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The distance to low-latitude negative-velocity clouds in the galactic anticenter will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1616649