ISOCAM images at 6.75 and 15 microns: the circumnuclear region of NGC 4321 (M 100)

Details ISOCAM images at 6.75 and 15 microns: the circumnuclear region of NGC 4321 (M 100) ISOCAM images at 6.75 and 15 microns: the circumnuclear region of NGC 4321 (M 100)

1997-11-13

arxiv.org/abs/astro-ph/9711149v1

Astronomy and Astrophysics

Astrophysics

Accepted for publication in A&A Letter. LaTeX using l-aa.sty. 4 pages, 1 Gif figure included (PS format at ftp://www-obs.cnr

Scientific paper

We present ISOCAM images (1.5"/px) in the LW2 (6.75 microns) and LW3 (15 microns) broad band filters of the circumnuclear starburst of NGC 4321 (M 100). A detailed comparison with the emission at other wavelengths (U, B, Halpha, and CO) is also presented. The nature and intensity of the mid-infrared emission is shown to be remarkably different from one star forming region to the next. For instance, star forming regions at the ends of the nuclear bar may contain enshrouded Wolf-Rayet stars.

Affiliated with

Also associated with

No associations

Rating

ISOCAM images at 6.75 and 15 microns: the circumnuclear region of NGC 4321 (M 100) 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 ISOCAM images at 6.75 and 15 microns: the circumnuclear region of NGC 4321 (M 100), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and ISOCAM images at 6.75 and 15 microns: the circumnuclear region of NGC 4321 (M 100) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-463950