Gaseous components along the line of sight to the supernova remnant N120

Details Gaseous components along the line of sight to the supernova remnant N120 Gaseous components along the line of sight to the supernova remnant N120

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26as...87..353v&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 87, no. 2, Feb. 1991, p. 353-360. In French.

Astronomy and Astrophysics

Astrophysics

2

Interstellar Gas, Line Of Sight, Magellanic Clouds, Supernova Remnants, Balmer Series, Emission Spectra, H Ii Regions, Red Shift

Scientific paper

As part of a two-dimensional study of energetic balance inside ring-like nebulae, 9 other nebulae or associated SNR-nebula were observed with the CIGALE equipment. After the SNRs N186D and N186E, the nebular complex N120 is being studied. It contains a large diffuse nebula with condensations, associated with a SNR identified by its nonthermal emission and X-ray emission. It is the largest identified SNR of the program, spreading over 2 x 1.5 arcmin. Three different gaseous layers are detected along the line of sight to N120.

Affiliated with

Also associated with

No associations

Rating

Gaseous components along the line of sight to the supernova remnant N120 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 Gaseous components along the line of sight to the supernova remnant N120, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gaseous components along the line of sight to the supernova remnant N120 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1315473