The Spatial Structure of the HH 30 Jet

Details The Spatial Structure of the HH 30 Jet The Spatial Structure of the HH 30 Jet

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..551r&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 551-552

Astronomy and Astrophysics

Astrophysics

1

Hh Objects: Individual: Hh 30, Hh 262

Scientific paper

New, deep, wide-field [SII] images of the HL Tauri region show the extended spatial structure of the HH 30 jet and counter-jet. At an angular distance of ˜ 300 arcsec toward the NE, the HH 30 jet ends in a group of scattered condensations. This previously undetected structure might correspond to a broken-up working surface. Our images also include HH 262, which is shown to have a previously undetected extended emission region.

Affiliated with

Also associated with

No associations

Rating

The Spatial Structure of the HH 30 Jet 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 Spatial Structure of the HH 30 Jet, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Spatial Structure of the HH 30 Jet will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1630476