SIMBAD references

2005PASP..117..931S - Publ. Astron. Soc. Pac., 117, 931-937 (2005/September-0)

A recurrence time versus orbital period relation for the Z Camelopardalis stars.

SHAFTER A.W., CANNIZZO J.K. and WAAGEN E.O.

Abstract (from CDS):

We examine AAVSO (American Association of Variable Star Observers) light curves of 16 Z Camelopardalis systems with measured orbital periods, with particular focus on intervals away from standstill. During these times, most of the systems display a sawtooth-like outburst behavior, with quiescent intervals comparable to the outburst durations. We report the discovery of a linear relation between the characteristic outburst period and orbital period for these systems, which is given by <Pout(days)≥62.0(±7.7)Porb(days)+2.41(±1.87).

Abstract Copyright: ∼

Journal keyword(s): Accretion, Accretion Disks - Stars: Binaries: Close - Stars: Individual: Constellation Name: RX Andromedae - stars: individual (KT Persei) - Stars: Individual: Constellation Name: TZ Persei - stars: individual (AM Cassiopeiae) - stars: individual (SV Canis Minoris) - Stars: Individual: Constellation Name: Z Camelopardalis - stars: individual (AT Cancri) - Stars: Individual: Constellation Name: SY Cancri - Stars: Individual: Constellation Name: AH Herculis - stars: individual (EM Cygni) - stars: individual (AB Draconis) - stars: individual (CN Orionis) - Stars: Individual: Constellation Name: UZ Serpentis - Stars: Individual: Constellation Name: HX Pegasi - Stars: Individual: Constellation Name: HL Canis Majoris - stars: individual (V426 Ophiuchi)

Simbad objects: 17

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