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The study of star clusters plays an important role in our understanding of the Universe since these systems are natural laboratories for testing theories of stellar dynamics and evolution. Particularly, globular clusters (GCs) are one of…

高能天体物理现象 · 物理学 2020-08-31 Diogo Belloni , Liliana E. Rivera Sandoval

I report the discovery of twenty-two new variable stars in the Northern Sky: eleven eclipsing, seven pulsating (one of which is suspected), three rotating, and one of unspecified type. Three already known variables (PT Lyr, [WM2007] 1157,…

太阳与恒星天体物理 · 物理学 2014-12-16 Riccardo Furgoni

Using XMM-Newton EPIC imaging data, we have detected 50 low-luminosity X-ray sources in the field of view of M 22, where 5 +/- 3 of these sources are likely to be related to the cluster. Using differential optical photometry, we have…

天体物理学 · 物理学 2016-08-30 N. A. Webb , D. Serre , B. Gendre , D. Barret , J. -P. Lasota , L. Rizzi

We have recently announced that the General Catalogue of Variable Stars enters the stage of its fifth, purely electronic edition (GCVS 5.1). Recently, we have incorporated a new, completely revised version for 1408 variable stars in the…

太阳与恒星天体物理 · 物理学 2018-07-25 N. N. Samus , E. N. Pastukhova , O. V. Durlevich , E. V. Kazarovets

The commissioning year of the Sloan Digital Sky Survey has demonstrated that many cataclysmic variables have been missed in previous surveys with brighter limits. We report the identification of 22 cataclysmic variables, of which 19 are new…

The search was performed for cataclysmic variable stars with outlying infrared magnitudes in USNO-B1.0 catalog. The selection was limited to objects in the Northern hemisphere with (B1-R1) < 1 and (R2-I) > 3.5. The search method is…

太阳与恒星天体物理 · 物理学 2015-05-30 D. V. Denisenko

The census of Galactic globular clusters (GCs) is still incomplete, and about ten new objects are supposed to await discovery, hidden behind the crowded and reddened regions of the Galactic bulge and disk. We investigated the nature of…

Cataclysmic variables (CVs) are compact binary systems in which a white dwarf accretes matter from a Roche-lobe-filling companion star. In this study, we searched for new CVs in the Milky Way in the Chandra Source Catalog v2.0,…

We present optical lightcurves, spectroscopy, and classification of five X-ray sources in the Chandra Galactic Bulge Survey [CXOGBS J174009.1-284725 (CX5), CXOGBS J173935.7-272935 (CX18), CXOGBS J173946.9-271809 (CX28), CXOGBS…

We present a multi-object optical spectroscopy follow-up study of X-ray sources in a field along the Galactic Plane (l=327.42 deg, b=2.26 deg) which is part of the Chandra Multi-wavelength Plane survey (ChaMPlane). We obtained spectra for…

高能天体物理现象 · 物理学 2015-06-03 Mathieu Servillat , J. Grindlay , M. van den Berg , J. Hong , P. Zhao , B. Allen

Dwarf novae in globular clusters seem to be rare with only 13 detections in the 157 known Galactic globular clusters. We report the identification of a new dwarf nova in M13, the 14th dwarf nova identified in a globular cluster to date.…

太阳与恒星天体物理 · 物理学 2015-05-27 Mathieu Servillat , N. A. Webb , F. Lewis , C. Knigge , M. van den Berg , A. Dieball , J. Grindlay

The aim of present work is extract and analyses the light curves of the stars in the field of two clusters, NGC 1960 and DOLIDZE 14. The photometric calibration is performed by comprehensive method of secondary standard transformation and…

太阳与恒星天体物理 · 物理学 2023-08-02 Gireesh C. Joshi

We compare the X-ray spectra and luminosities, in the 2-8 keV band, of known and suspected cataclysmic variables (CVs) in different environments, assessing the nature of these source populations. These objects include nearby CVs observed…

天体物理学 · 物理学 2009-06-23 Craig O. Heinke , Ashley J. Ruiter , Michael P. Muno , Krzysztof Belczynski

We examined 134 Chandra observations of the population of X-ray sources associated with globular clusters (GCs) in the central region of M31. These are expected to be X-ray binary systems (XBs), consisting of a neutron star or black hole…

高能天体物理现象 · 物理学 2015-06-04 R. Barnard , M. Garcia , S. S. Murray

We carry out a photometric search for new cataclysmic variable stars (CVs), with the goal of identification for candidates of AR~Scorpii-type binary systems. We select GAIA sources that are likely associated with unidentified X-ray sources,…

太阳与恒星天体物理 · 物理学 2022-09-14 J. Takata , X. F. Wang , A. K. H. Kong , J. Mao , X. Hou , C. -P. Hu , L. C. -C. Lin , K. L. Li , C. Y. Hui

The VVV is currently surveying the central regions of the Milky Way at near-infrared wavelengths, including 36 known Galactic globular clusters. We already have data in several filters to generate their color-magnitude diagrams. We also…

We report the detection of variable stars within a 11.5' x 11.5' region near the Galactic centre (GC) that includes the Arches and Quintuplet clusters, as revealed by the VISTA Variables in the Via Lactea (VVV) survey. There are 353 sources…

太阳与恒星天体物理 · 物理学 2018-11-28 C. Navarro Molina , J. Borissova , M. Catelan , P. W. Lucas , N. Medina , C. Contreras Pena , R. Kurtev , D. Minniti

We present new BVI photometry of the globular cluster NGC 6981 (M72), based mostly on ground-based CCD archive images. We present a new color-magnitude diagram (CMD) that reaches almost four magnitudes below the turn-off level. We performed…

星系天体物理 · 物理学 2015-06-17 P. Amigo , P. B. Stetson , M. Catelan , M. Zoccali , H. A. Smith

We present low resolution optical spectroscopy for six cataclysmic variable candidates and the old nova V888 Cen. We confirm the classification as cataclysmic variable for LB 9963 and FQ Mon, while the other four candidates turn out to be…

天体物理学 · 物理学 2009-11-11 L. Schmidtobreick , L. Galli , A. Whiting , C. Tappert , A. J. Carver

Every massive globular cluster (GC) is expected to harbour a significant population of cataclysmic variables (CVs). In this review, I first explain why GC CVs matter astrophysically, how many and what types are theoretically predicted to…

太阳与恒星天体物理 · 物理学 2012-02-13 Christian Knigge
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