Mid-infrared images of W75N (Persi+, 2006)

Details Mid-infrared images of W75N (Persi+, 2006) Mid-infrared images of W75N (Persi+, 2006)

Feb 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..34450971p&link_type=abstract

VizieR On-line Data Catalog: J/A+A/445/971. Originally published in: 2006A&A...445..971P

Astronomy and Astrophysics

Astronomy

H Ii Regions, Ysos, Infrared Sources

Scientific paper

Mid-infrared images between 8.7 and 18.7um of W75N were taken during three observing runs on September 2000, November 2001 and September 2003 with the mid-infrared camera CID on the 2.1 m telescope of the Observatorio Astronomico Nacional at San Pedro Martir, Baja California, Mexico.
The images at 3.6, 4.5, 5.8 and 8.0um of W75N presented here are sections of the original IRAC images of the star forming region DR21 observed during the science verification period of the Spitzer satellite.
(1 data file).

Affiliated with

Also associated with

No associations

Rating

Mid-infrared images of W75N (Persi+, 2006) 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 Mid-infrared images of W75N (Persi+, 2006), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mid-infrared images of W75N (Persi+, 2006) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1466727