STIS Observation of UV High-Velocity Interstellar Lines in the Carina Nebula

Details STIS Observation of UV High-Velocity Interstellar Lines in the Carina Nebula STIS Observation of UV High-Velocity Interstellar Lines in the Carina Nebula

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hst..prop.7137w&link_type=abstract

HST Proposal ID #7137

Computer Science

Hst Proposal Id #7137

Scientific paper

To demonstrate the highest STIS resolution in the UV, the star CPD-59D2603, located in the Carina Nebula and known from optical and IUE observations to display spectacular interstellar-line velocity structure over a range of at least 340 km/sec, will be observed with the H echelles. It is expected that STIS will resolve many more velocity components than previously observed in these intricate profiles. The phenomenon is likely due to interaction between the massive stellar winds and the surrounding interstellar material, and it is probably related to the diffuse X-ray emission from the region.

Affiliated with

Also associated with

No associations

Rating

STIS Observation of UV High-Velocity Interstellar Lines in the Carina Nebula 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 STIS Observation of UV High-Velocity Interstellar Lines in the Carina Nebula, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and STIS Observation of UV High-Velocity Interstellar Lines in the Carina Nebula will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-895052