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Related papers: Variable stars in Stellar Systems

200 papers

We have used DOLORES at the TNG to obtain B,V time series photometry of NGC 2419, one of the most distant and bright clusters in the Galactic halo. These data will be used to study its variable star population in order to check whether the…

Recent high-resolution observations of the central region of Galactic globular clusters have shown the presence of a large variety of exotic stellar objects whose formation and evolution may be strongly affected by dynamical interactions.…

Astrophysics · Physics 2016-08-30 Francesco R. Ferraro

Globular cluster systems exhibit a bewildering variety of characteristics. No single scenario appears to be able to account for the wide range of specific globular cluster frequencies that are observed in galaxies of various types. The…

Astrophysics · Physics 2009-10-31 Sidney van den Bergh

We present the first results of our variability survey for the globular cluster NGC 362. We found numerous variable stars in the field including 23 RR Lyr stars, 4 eclipsing binaries and 5 other pulsating stars. Four of the RR Lyr ae stars…

Astrophysics · Physics 2010-12-09 P. Székely , L. L. Kiss , B. Csák , A. Derekas , T. R. Bedding , K. Szatmáry

Developments of this far-reaching research field are summarized from an observational point of view, mentioning important and interesting phenomena discovered recently by photometry of stellar oscillations of any kind. A special emphasis is…

Solar and Stellar Astrophysics · Physics 2014-04-08 L. Szabados

The stellar evolution theory of massive stars remains uncalibrated with high-precision photometric observational data mainly due to a small number of luminous stars that are monitored from space. Automated all-sky surveys have revealed…

Solar and Stellar Astrophysics · Physics 2017-02-08 Jaan Laur , Indrek Kolka , Tõnis Eenmäe , Taavi Tuvikene , Laurits Leedjärv

Star clusters are fundamental units of stellar feedback and unique tracers of their host galactic properties. In this review, we will first focus on their constituents, i.e.\ detailed insight into their stellar populations and their…

Surveys of pulsating stars in the inner Galaxy have been very limited, but recent large-scale surveys are rapidly bringing us new samples of various kinds of variable stars and new insights into stellar populations therein. Because of the…

Solar and Stellar Astrophysics · Physics 2018-08-22 Noriyuki Matsunaga

In this paper I present an overview of the main observational properties of a special class of exotic objects (the so-called Blue Straggler Stars, BSSs) in Galactic Globular Clusters (GCs). The BSS specific frequency and their radial…

Astrophysics of Galaxies · Physics 2017-08-23 Francesco R. Ferraro

In this chapter I review the recent developments regarding the study of Blue Stragglers (BSS) in dwarf galaxies. The loose density environment of dwarf galaxies resembles that of the Galactic Halo, hence it is natural to compare their…

Solar and Stellar Astrophysics · Physics 2015-06-22 Yazan Momany

Dwarf galaxies in the local group provide a unique astrophysical laboratory. Despite their proximity some of these systems still lack a reliable distance determination as well as studies of their stellar content and star formation history.…

Astrophysics · Physics 2007-05-23 Jan Snigula , Claus Goessl , Ulrich Hopp , Heinz Barwig

We obtained a series of more than two hundred R-band CCD images for the crowded central (115"x77") region of the metal-poor globular cluster M15 with an angular resolution of 0.5"-0.9" in most images. Optimal image subtraction was used to…

Astrophysics · Physics 2009-11-10 Alexander P. Zheleznyak , Valery V. Kravtsov

Recent progress in our knowledge of stellar populations in local dwarf spheroidal galaxies is briefly discussed. A few results are summarized including wide field observations of stellar populations and their spatial variations, studies of…

Astrophysics · Physics 2009-11-11 Enrico V. Held

The central part of the globular cluster NGC 288 was surveyed in a search for short-period variable stars. We obtained the V-band light curves for 4 SX Phe stars and 2 RR Lyrae variables, five of which are new discoveries. All SX Phe stars…

Astrophysics · Physics 2007-05-23 J. Kaluzny

We report the discovery of a variable blue straggler in the core of the globular cluster M5, based on a 12-hour long series of images obtained with the Planetary Camera aboard the Hubble Space Telescope. In addition, we present the light…

Astrophysics · Physics 2009-10-30 L. Drissen , M. M. Shara

A sample of 86 contact binary systems in 14 globular clusters with available color index data in (B-V) or in (V-I) has been analyzed. At least one third of all systems are numerous foreground Galactic Disk projections over long lines of…

Astrophysics · Physics 2009-10-31 Slavek M. Rucinski

Globular clusters are among the most congested stellar systems in the Universe. Internal dynamical evolution drives them toward states of high central density, while simultaneously concentrating the most massive stars and binary systems in…

Solar and Stellar Astrophysics · Physics 2015-06-22 Stephen L. W. McMillan

In the last decade we witness an advent of new types of dwarf stellar systems in cluding ultra-compact dwarfs, ultra-faint dwarf spheroidals, and exotic globular clusters, breaking the old simple paradigm for dwarf galaxies and globular…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-20 Myung Gyoon Lee , Sungsoon Lim , Hong Soo Park , Ho Seong Hwang , Narae Hwang

Blue Straggler stars are present in all the properly observed Globular Clusters. They mimic a rejuvenated stellar population and their existence has been a puzzle for many years. We performed an extensive spectroscopic survey of the surface…

Solar and Stellar Astrophysics · Physics 2013-01-16 Loredana Lovisi , Alessio Mucciarelli , Barbara Lanzoni , Francesco R. Ferraro , Emanuele Dalessandro

CCD photometry in the V band is presented for 7 field RR Lyrae stars selected from a sample of eight variables which, according to data collected in the literature, are expected to be {\it ab}-type pulsators, to have short periods and hence…

Astrophysics · Physics 2015-06-24 G. Clementini , M. Tosi , A. Bragaglia , R. Merighi , C. Maceroni