Dwarf Nova V1040 Centauri and Variable Stars in its Vicinity

被引：0

作者：

Rutkowski, A. ^{[1
]}

Pietrukowicz, P. ^{[2
]}

Olech, A. ^{[3
]}

Ak, T. ^{[4
]}

Zloczewski, K. ^{[3
]}

Poleski, R. ^{[2
]}

Tappert, C. ^{[5
]}

Eker, Z. ^{[1
,6
]}

机构：

[1] Akdeniz Univ, TUBITAK Natl Observ, TR-07058 Antalya, Turkey

[2] Univ Warsaw Observ, PL-00478 Warsaw, Poland

[3] Polish Acad Sci, Nieolaus Copernicus Astron Ctr, PL-00716 Warsaw, Poland

[4] Istanbul Univ, Fac Sci, Dept Astron & Space Sci, TR-34119 Istanbul, Turkey

[5] Univ Valparaiso, Dept Fis & Astrofis, Valparaiso, Chile

[6] Akdeniz Univ, Dept Phys, Fac Scince & Art, TR-07058 Antalya, Turkey

来源：

ACTA ASTRONOMICA | 2011年 / 61卷 / 04期

基金：

欧洲研究理事会;

关键词：

Accretion; accretion disks; novae; cataclysmic variables; Stars: oscillations (including pulsations); Stars:; individual:; V1040; Cen; RX J1155.4-5641; AAVSO; 1150-56; 2MASS J11552726-5641561; ALPHA-SELECTED SAMPLE; CATACLYSMIC VARIABLES; EXPERIMENT CURVE; CCD PHOTOMETRY; URSAE MAJORIS; SUPERHUMPS; SUPEROUTBURST;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the results of a photometric campaign of the dwarf nova V1040 Cen. The light curve shows two normal outbursts with recurrence time approximate to 40 days and amplitude approximate to 2.5 mag. Quiescence data show oscillations with periods in the range approximate to 0.1 days (2.4 h) to approximate to 0.5 days (12 h) of unknown origin. We measured the orbital period of V1040 Cen to be P(orb) = 0.060458(80) days (1.451 +/- 0.002 h). Based on the M(V)-P(orb) relation we found the distance of V1040 Cen to be 137 +/- 31 pc. In this paper we also report the detection of eleven new variable stars in the field of the monitored dwarf nova.

引用

页码：345 / 357

页数：13

共 11 条

[1] V485 Centauri: A dwarf nova with a 59(m) orbital period
Augusteijn, T
vanderHooft, F
deJong, JA
vanParadijs, J
ASTRONOMY & ASTROPHYSICS, 1996, 311 (03) : 889 - 900
[2] A 59M PHOTOMETRIC PERIOD IN THE DWARF NOVA V485 CENTAURI
AUGUSTEIJN, T
VANKERKWIJK, MH
VANPARADIJS, J
ASTRONOMY & ASTROPHYSICS, 1993, 267 (02) : L55 - L58
[3] V803 Centauri: Helium dwarf nova mimicking a WZ Sge-type superoutburst
Kato, T
Stubbings, R
Monard, B
Butterworth, ND
Bolt, G
Richards, T
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2004, 56 (01) : S89 - S98
[4] Dwarf nova-type cataclysmic variable stars are significant radio emitters
Coppejans, Deanne L.
Kording, Elmar G.
Miller-Jones, James C. A.
Rupen, Michael P.
Sivakoff, Gregory R.
Knigge, Christian
Groot, Paul J.
Woudt, Patrick A.
Waagen, Elizabeth O.
Templeton, Matthew
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2016, 463 (02) : 2229 - 2241
[5] The nature of V359 Centauri revealed: New long-period SU UMa-type dwarf nova
Kato, T
Stubbings, R
Nelson, P
Santallo, R
Ishioka, R
Uemura, M
Sumi, T
Muraki, Y
Kilmartin, P
Bond, I
Noda, S
Yock, P
Hearnshaw, JB
Monard, B
Yamaoka, H
ASTRONOMY & ASTROPHYSICS, 2002, 395 (02) : 541 - 548
[6] High speed photometry of faint cataclysmic variables - VI. Car2, V1040 Cen, Hα 075648, IL Nor (Nova Nor 1893), HS Pup (Nova Pup 1963), SDSS J2048-06, CSS 081419-005022 and CSS 112634-100210
Woudt, Patrick A.
Warner, Brian
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2010, 403 (01) : 398 - 404
[7] Spectral evolution of the nova V2468 Cygni: asymmetric and variable profiles of its emission lines
Iijima, T.
Naito, H.
ASTRONOMY & ASTROPHYSICS, 2011, 526
[8] The Heating and Pulsations of V386 Serpentis after Its 2019 Dwarf Nova Outburst
Szkody, Paula
Godon, Patrick
Gansicke, Boris T.
Kafka, Stella
Castillo, Odette F. T.
Bell, Keaton J.
Cho, P. B.
Sion, Edward M.
Kumar, Praphull
Townsley, Dean M.
Vanderbosch, Zach
Winget, Karen I.
Olde Loohuis, Claire J.
ASTROPHYSICAL JOURNAL, 2021, 914 (01)
[9] Cataclysmic and close binaries in star clusters. V. Erupting dwarf novae, faint blue stars, X-ray sources, and the classical nova in the core of M80
Shara, MM
Hinkley, S
Zurek, DR
ASTROPHYSICAL JOURNAL, 2005, 634 (02) : 1272 - 1285
[10] Infrared photometry of the dwarf nova V2051 Ophiuchi - II. The quiescent accretion disc and its spiral arms
Baptista, Raymundo
Wojcikiewicz, Eduardo
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2020, 492 (01) : 1154 - 1163

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