M87'S Jet, Nucleus, and Hot Corona (fos no. 12): Cycle 4 Observations

Details M87'S Jet, Nucleus, and Hot Corona (fos no. 12): Cycle 4 Observations M87'S Jet, Nucleus, and Hot Corona (fos no. 12): Cycle 4 Observations

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5122f&link_type=abstract

HST Proposal ID #5122

Physics

Hst Proposal Id #5122 Quasars &Amp, Agn

Scientific paper

WF/PC narrow band images of M87 will be used to isolate emission line regions near the nucleus and jet. FOS spectra of these clouds will be used to i) map the velocity field near the nucleus, ii) understand physical conditions and ionization mechanisms in these clouds, and iii) measure chemical composition of the clouds. FOS spectra of the stellar nucleus and synchotron knots in the jet will be used to establish long-base-line spectral indices and to look for spectral features. Long exposure ultraviolet spectra of the nucleus and jet will be used to look for absorption lines from M87's hot corona.

Affiliated with

Also associated with

No associations

Rating

M87'S Jet, Nucleus, and Hot Corona (fos no. 12): Cycle 4 Observations 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 M87'S Jet, Nucleus, and Hot Corona (fos no. 12): Cycle 4 Observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and M87'S Jet, Nucleus, and Hot Corona (fos no. 12): Cycle 4 Observations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1255346