Hostname: page-component-84b7d79bbc-dwq4g Total loading time: 0 Render date: 2024-07-30T06:20:54.394Z Has data issue: false hasContentIssue false
  • English
  • Français

V1493 AQL an Extremely Distant Nova?

Published online by Cambridge University Press:  22 February 2018

A. Dobrotka ,
A. Retter ,
L. Hric ,
R. Novak ,
O. Shemmer  and
Y. Lipkin
A. Dobrotka
Affiliation:
Departement of Physics, Faculty of Materials Science and Technology,Slovak University of Technology in Bratislava, Paulinska 16, Trnava 917 24, The Slovak Republic (dobrotka@mtf.stuba.sk)
A. Retter
Affiliation:
School of Physics, University of Sydney, 2006, Australia (e-mail: retter@physics.nsyd.edu.au)
L. Hric
Affiliation:
Astronomical Institute of the Slovak Academy of Sciences, 059 60 Tatranská Lomnica, The Slovak Republic (e-mail: hric@ta3.sk)
R. Novak
Affiliation:
Nicholas Copernicus Observatory and Planetarium in Brno, Kravi hora 2, 616 00 Brno, Czech Republic (e-mail: novak@hvezdarna.cz)
O. Shemmer
Affiliation:
The Raymond and Beverly Sackler faculty of exact sciences, school of physics and astronomy and the Wise Observatory, Tel-Aviv University, Israel (e-mail: ohad@wise.tau.ac.il.yiftah@wise.tau.ac.il)
Y. Lipkin
Affiliation:
The Raymond and Beverly Sackler faculty of exact sciences, school of physics and astronomy and the Wise Observatory, Tel-Aviv University, Israel (e-mail: ohad@wise.tau.ac.il.yiftah@wise.tau.ac.il)

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Analysis of CCD photometry performed during 12 nights and the estimate of the distance based on the light curve is presented. The photometric data is modulated with a period of 3.7 h, which we interpret as the orbital period above the period gap distribution of cataclysmic variables. The VSNET light curve combined with data from IAU Circulars suggests a distance of 4.5±0.4 kpc based on t2/t3 time estimates. Two spectra 11 days after the maximum were taken. The expansion velocity of the envelope was derived to be 1658±62 km s–1.

Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004 , pp. 236
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

References

Arkhipova, V.P., Burlak, M.A., Esipov, V.F., 2002, AL 28, 100 Google Scholar
Bonifacio, P., Selvelli, P.L., Caffau, E., 2000, A&A 356, L53 Google Scholar
Nakano, S.. Tago, A., 1999, IAUC 7223Google Scholar
Tomov, T., Moro, D., Munari, U., 1999. IAUC 7225Google Scholar