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相关论文: Distance Scale, Variable Stars and Stellar Populat…

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We briefly review our photometric and spectroscopic study of RR Lyrae variable stars in the bar of the Large Magellanic Cloud (LMC), that allowed us to reconcile the so-called "short" and "long" distance moduli of the LMC on the value…

Results are presented of a study of the variable star populations in the dwarf spheroidal galaxy Leo I and in the dwarf irregular galaxy NGC 6822, based on time series photometry obtained with the Wide Field Imager of the 2.2 m ESO/MPI…

天体物理学 · 物理学 2007-05-23 L. Baldacci , F. Matonti , L. Rizzi , G. Clementini , E. V. Held , Y. Momany , L. Di Fabrizio , I. Saviane

We present the first results of a variable star search in the field and in the globular clusters of the Fornax dwarf spheroidal galaxy. Variable stars were identified using the Image Subtraction Technique (Alard 2000) on time-series data…

Results are presented on a study of the short period variable stars in the dwarf irregular galaxy NGC6822. We observed an almost uniformely populated classical instability strip from the Horizontal Branch up to the Classical Cepheids…

天体物理学 · 物理学 2007-05-23 L. Baldacci , L. Rizzi , G. Clementini , E. V. Held , .

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.…

天体物理学 · 物理学 2007-05-23 Jan Snigula , Claus Goessl , Ulrich Hopp , Heinz Barwig

We report the discovery of a large number of short-period variable stars in the dwarf irregular galaxy NGC6822, based on deep time-series imaging carried out with the ESO Very Large Telescope. In particular, we found a modest population of…

天体物理学 · 物理学 2009-11-07 G. Clementini , E. V. Held , L. Baldacci , L. Rizzi

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.…

天体物理学 · 物理学 2007-05-23 C. A. Goessl , J. Snigula , U. Hopp

We present a search for variable stars in the Fornax dwarf galaxy covering an area of 1/2 a square degree. We have ~30 epochs of VI data. We found and determined periods for more than 500 RR Lyrae, 17 anomalous Cepheids, 6 Population II…

天体物理学 · 物理学 2009-11-07 D. Bersier , P. R. Wood

This paper summaries the status of a large project to improve distance scales of various classes of variable stars. This is being carried out by a large group in Cape Town, Japan, England and the USA. The results are illustrated by giving…

天体物理学 · 物理学 2008-06-19 Michael W. Feast

We present a comprehensive analysis of the variable stars projected on the field of the Galactic bulge globular cluster NGC 6522, offering valuable insights into their characteristics. Using proper motions from Gaia DR3, we aim to…

太阳与恒星天体物理 · 物理学 2023-10-26 A. Arellano Ferro , Z. Prudil , M. A. Yepez , I. Bustos Fierro , A. Luna

We discuss in detail the pulsation properties of variable stars in globular clusters (GCs) and in Local Group (LG) dwarf galaxies. Data available in the literature strongly support the evidence that we still lack a complete census of…

天体物理学 · 物理学 2007-05-23 Giuseppe Bono , Silvia Petroni , Marcella Marconi

We present a new study of the variable star population in globular cluster 5 of the Fornax dwarf spheroidal galaxy, based on B and V time series photometry obtained with the MagIC camera of the 6.5 m Magellan Clay telescope and…

The new data for Cepheids and RR Lyrae stars of the Optical Gravitational Lensing Experiment (OGLE-III) survey allow us to study the three-dimensional distribution of stars corresponding to young (a few tens to a few hundreds of millions of…

星系天体物理 · 物理学 2015-06-05 Raoul Haschke , Eva K. Grebel , Sonia Duffau

This is the second in a series of papers studying the variable stars in Large Magellanic Cloud globular clusters. The primary goal of this series is to study how RR Lyrae stars in Oosterhoff-intermediate systems compare to their…

太阳与恒星天体物理 · 物理学 2015-06-11 Charles A. Kuehn , Horace A. Smith , Marcio Catelan , Barton J. Pritzl , Nathan De Lee , Jura Borissova

Variable stars have been identified for the first time in Fornax 4, the globular cluster located near the center of the Fornax dwarf spheroidal galaxy. By applying the image subtraction technique to B,V time series photometry obtained with…

Dwarf galaxies in the local group provide a unique astrophysical laboratory. In particular, they allow us to probe pulsating (and other) variable stars in low-metallicity environments with abundances below that of the SMC. Our observing…

天体物理学 · 物理学 2007-05-23 J. Snigula , C. A. Goessl , U. Hopp

We present new observations of Sextans and Leo I dwarf galaxies, that provide new insight on their stellar populations. The large sample of stars measured in Sextans allowed us to obtain a reliable estimate of the metal content of this…

天体物理学 · 物理学 2007-05-23 L. Rizzi , E. V. Held , I. Saviane , Y. Momany , G. Clementini , G. Bertelli

This is the third in a series of papers studying the variable stars in old globular clusters in the Large Magellanic Cloud. The primary goal of this series is to look at how the characteristics and behavior of RR Lyrae stars in…

(Abridged) We have surveyed four globular clusters in the Fornax dwarf galaxy for RR Lyrae stars, using archival HST observations. We identify 197 new RR Lyrae stars in these four clusters. Despite the short observational baseline, we…

天体物理学 · 物理学 2009-11-10 A. D. Mackey , G. F. Gilmore

The near and mid-infrared characteristics of large amplitude, Mira, variables in Local Group dwarf irregular galaxies (LMC, NGC 6822, IC 1613, Sgr dIG) are described. Two aspects of these variables are discussed. First, the short period (P…

星系天体物理 · 物理学 2017-11-27 Patricia A. Whitelock
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