Neutral hydrogen in the M96 group - Evidence for a giant intergalactic ring

Details Neutral hydrogen in the M96 group - Evidence for a giant intergalactic ring Neutral hydrogen in the M96 group - Evidence for a giant intergalactic ring

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...288l..33s&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 288, Jan. 15, 1985, p. L33-L35.

Astronomy and Astrophysics

Astrophysics

50

Cosmic Gases, Hydrogen Clouds, Intergalactic Media, Astronomical Models, Mass To Light Ratios, Orbits, Radial Velocity, Ring Structures

Scientific paper

Further Arecibo observations of the region around the intergalactic cloud in Leo have uncovered several smaller isolated clouds. Altogether, the H I lies primarily along a 200 kpc diameter ring around the galaxies M105 (E0) and NGC 3384 (SB0). The radial velocities around the ring follow a Keplerian orbit pattern with a period of 4×109yr.

Affiliated with

Also associated with

No associations

Rating

Neutral hydrogen in the M96 group - Evidence for a giant intergalactic ring 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 in the M96 group - Evidence for a giant intergalactic ring, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Neutral hydrogen in the M96 group - Evidence for a giant intergalactic ring will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-925489