Outburst and quiescence observations of the Dwarf Nova V101 in the globular Cluster M5

Details Outburst and quiescence observations of the Dwarf Nova V101 in the globular Cluster M5 Outburst and quiescence observations of the Dwarf Nova V101 in the globular Cluster M5

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987aj.....94..357s&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 94, Aug. 1987, p. 357-359, 535.

Astronomy and Astrophysics

Astronomy

17

Binary Stars, Dwarf Novae, Globular Clusters, Stellar Spectrophotometry, Variable Stars, Data Reduction, Light Curve, Orbital Elements

Scientific paper

The authors have observed the dwarf nova V101 towards the globular cluster M5 through most of an eruption, and during quiescence. Assuming it to be a member of the cluster, V101 reached MB ≅ +4.3 at maximum and MB ≡ +7.6 at minimum, in good agreement with determinations for field dwarf novae. The outburst rise and fall times and total duration imply a long orbital period (≡11 hr) and possibly an evolved secondary. This hypothesis is consistent with the red continuum of V101 seen in the spectrum of Margon et al. (1981).

Affiliated with

Also associated with

No associations

Rating

Outburst and quiescence observations of the Dwarf Nova V101 in the globular Cluster M5 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 Outburst and quiescence observations of the Dwarf Nova V101 in the globular Cluster M5, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Outburst and quiescence observations of the Dwarf Nova V101 in the globular Cluster M5 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1339740