Spatially resolved echellette spectroscopy of low-excitation Herbig-Haro objects and its interpretation

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

51

Astronomical Spectroscopy, Echelette Gratings, Herbig-Haro Objects, Line Spectra, Spatial Resolution, Stellar Winds, Forbidden Transitions, H Beta Line, Iron, Near Infrared Radiation, Visible Spectrum

Scientific paper

Spatially resolved spectra of the low-excitation Herbig-Haro (HH) objects HH 7, HH 11, HH 43 B, and HH 43 C and of the high-excitation object HH 43 A, obtained with the 'echellette' spectrograph at the 3.5-m telescope and the coude spectrograph at the 2.2-m telescope of the Calar Alto Observatory, were studied in the spectral range between 3700 and 10,000 A. A considerable number of new lines were detected in all five objects. The spatial distributions of the intensities and the radial velocities were investigated. Using the forbidden line ratios, the spatial distributions of the electron temperature and density were determined.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Spatially resolved echellette spectroscopy of low-excitation Herbig-Haro objects and its interpretation 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 Spatially resolved echellette spectroscopy of low-excitation Herbig-Haro objects and its interpretation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spatially resolved echellette spectroscopy of low-excitation Herbig-Haro objects and its interpretation will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1560472

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.