A possible orbital period for the dwarf nova V1101 Aql

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dc.creatorMasetti, Nicola
dc.creatorDella Valle, Massimo
dc.date1997-11-11
dc.date.accessioned2026-07-07T02:25:01Z
dc.date.available2026-07-07T02:25:01Z
dc.descriptionWe have performed a Discrete Fourier Transform on 136 CCD B, V and R frames of the Z Cam-type dwarf nova V1101 Aql. Our analysis indicates as possible orbital period P_orb =3.46 hours, though we cannot exclude the alias at 4.00 hours. We estimate the distance to the system to be about 300 pc. We possibly discovered a bright bow-shaped nebulosity around the object.
dc.description8 pages, 8 .ps figures, A&A LaTeX style file l-aa.sty version 3.0. Accepted for publication by Astronomy and Astrophysics, Main Journal
dc.identifierhttps://arxiv.org/abs/astro-ph/9711115
dc.identifierhttp://arxiv.org/abs/astro-ph/9711115
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11777
dc.subjectAstrophysics
dc.titleA possible orbital period for the dwarf nova V1101 Aql
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