Optical spectroscopy of the jet in V Hydrae.

Details Optical spectroscopy of the jet in V Hydrae. Optical spectroscopy of the jet in V Hydrae.

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.248..479l&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. Vol. 248, No. 3, p. 479 - 482

Astronomy and Astrophysics

Astronomy

6

Scientific paper

Spectra of the 3600-4700 Å region of the spectrum of the carbon star V Hya reveal a rich emission-line spectrum similar to those found in objects where shock waves occur. A radial velocity of -155 km s-1 relative to the star indicates that we see the nearer lobe of the bipolar jet already known in V Hya. The unusually strong violet continuum and the absorption in the higher Balmer lines, which yield a radial velocity slightly different from that of the carbon star, may arise in the hypothetical companion.

Affiliated with

Also associated with

No associations

Rating

Optical spectroscopy of the jet in V Hydrae. 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 Optical spectroscopy of the jet in V Hydrae., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Optical spectroscopy of the jet in V Hydrae. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1318184