The very slow nova He 3-558

Details The very slow nova He 3-558 The very slow nova He 3-558

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...200..694h&link_type=abstract

Astrophysical Journal, vol. 200, Sept. 15, 1975, pt. 1, p. 694-697. Research supported by the University of Michigan

Astronomy and Astrophysics

Astrophysics

3

Light Curve, Novae, Stellar Spectra, Spectral Line Width, Spectrum Analysis, Stellar Luminosity

Scientific paper

The emission-line object He 3-558 has been found to be a very slow nova
which rose to maximum brightness in 1948 and is probably still fading.
Its spectrum and light curve are described, and a distance of 3.5 kpc is
derived. No sign of an earlier outburst was found in the Harvard
collection of photographs.

Affiliated with

Also associated with

No associations

Rating

The very slow nova He 3-558 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 The very slow nova He 3-558, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The very slow nova He 3-558 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-909405