A POSSIBLE ORBITAL PERIOD FOR THE DWARF NOVA V1101 AQ1

Authors
MASETTI N DELLAVALLE M
Citation
N. Masetti et M. Dellavalle, A POSSIBLE ORBITAL PERIOD FOR THE DWARF NOVA V1101 AQ1, Astronomy and astrophysics, 331(1), 1998, pp. 187-192
Citations number
19
Categorie Soggetti
Astronomy & Astrophysics
Journal title
Astronomy and astrophysics → ACNP
ISSN journal
00046361
Volume
331
Issue
1
Year of publication
1998
Pages
187 - 192
Database
ISI
SICI code
0004-6361(1998)331:1<187:APOPFT>2.0.ZU;2-U
Abstract
We have performed a Discrete Fourier Transform on 136 CCD B, V and R f rames of the Z Cam-type dwarf nova V1101 Aql. Our analysis indicates a s possible orbital period P-orb = 3(h).46, though we cannot exclude th e alias at 4(h).00. We estimate the distance to the system to be about 300 pc. We possibly discovered a bright bow-shaped nebulosity around the object.