SIMBAD references

1996PASP..108..408W - Publ. Astron. Soc. Pac., 108, 408-411 (1996/May-0)

The spectrum of Wakuda's eruptive star near the time of outburst.

WALLERSTEIN G.

Abstract (from CDS):

We have made complete wavelength measurements and line identifications for the star discovered by Wakuda to have risen to magnitude 10.5 about one year before our observation on 3 April 1994. Wavelength coverage was from 4900 to 8800A. The spectrum is that of a "shell" with many emission lines of singly ionized metals. The systemic velocity is near +63.5 km s^-1, which transforms to +76 km s^-1 with respect to the local standard of rest indicating that Wakuda's star is a disk object, as are most symbiotic objects. If classified as a nova its distance indicates that it belongs to the Galactic bulge population.

Abstract Copyright:

Journal keyword(s): Stars

Simbad objects: 5

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:1996PASP..108..408W and select 'bookmark this link' or equivalent in the popup menu


2020.10.20-09:16:09

© Université de Strasbourg/CNRS

    • Contact