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相关论文: UBVRI photometric comparison sequences for symbiot…

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We present accurate UBVRI photometric comparison sequences around 20 symbiotic stars. The sequences extend over wide brightness and color ranges, and are suited to cover quiescence as well as outburst phases. The sequences are intended to…

天体物理学 · 物理学 2009-10-31 A. Henden , U. Munari

Deep, wide-range and accurate UBVRI photometric sequences have been established around more than 80 symbiotic stars, to assist current photometry as well as measurement of old photographic plates. Sequences for 40 symbiotic stars have…

天体物理学 · 物理学 2007-05-23 Ulisse Munari , Arne Henden

We present a multi-epoch, accurate UBVRcIc photometric catalog of 83 symbiotic stars and related objects, measured while calibrating the Henden and Munari (2000, 2001, 2006) photometric sequences around them. The vast majority of the…

太阳与恒星天体物理 · 物理学 2009-02-27 A. Henden , U. Munari

We present a new catalogue of symbiotic stars. In our list we include 188 symbiotic stars as well as 28 objects suspected of being symbiotic. For each star, we present basic observational material: coordinates, V and K magnitudes,…

天体物理学 · 物理学 2009-10-31 K. Belczynski , J. Mikolajewska , U. Munari , R. J. Ivison , M. Friedjung

We present results from a continuing campaign to secure deep multi-colour CCD sequences for photometric calibration in UK Schmidt fields with galactic latitudes |b|>50deg. In this paper we present UBVR photometry in 12 fields and BR…

天体物理学 · 物理学 2009-10-31 Scott M. Croom , A. Ratcliffe , Q. A. Parker , T. Shanks , B. J. Boyle , R. J. Smith

A new survey of star clusters in the South-West field of the M31 disk based on the high resolution Subaru Suprime-Cam observations is presented. The UBVRI aperture CCD photometry catalog of 285 objects (V < 20.5; 169 of them identified for…

天体物理学 · 物理学 2009-06-23 D. Narbutis , V. Vansevicius , K. Kodaira , A. Bridzius , R. Stonkute

We study the capability of the UBVRI photometric system to quantify star clusters in terms of age, metallicity, and color excess by their integrated photometry. The well known age-metallicity-extinction degeneracy was analyzed for various…

天体物理学 · 物理学 2008-11-26 D. Narbutis , A. Bridzius , R. Stonkute , V. Vansevicius

UBVRI photoelectric observations have been made of 109 stars around the sky, centered more or less at -50 degrees declination. The majority of the stars fall in the magnitude range 10.4 < V < 15.5 and in the color index range -0.33 < (B -…

天体物理学 · 物理学 2010-11-05 Arlo U. Landolt

We present time-series uvby-beta photometry of 41 classical Cepheid stars. A brief discussion of the comparison between the presented data and previous photometric data has been done.

太阳与恒星天体物理 · 物理学 2010-07-05 J. H. Peña , A. Arellano Ferro , R. Peña-Miller , M. Alvarez , Y. Rosas , H. , García , G. Muñoz , B. Vargas , J. P. Sareyan , C. A. Guerrero , A. Rentería

The results from work done to extend the Johnson-Cousins BVRI photometric standard sequence to faint levels of V ~ 21 mag in compact fields is presented. Such calibration and extension of sequences is necessary to fill a calibration gap, if…

天体物理学 · 物理学 2009-11-10 A. Saha , A. E. Dolphin , F. Thim , B. Whitmore

Based on 13 nights of observations of four fields in NGC 300, we have set up an extensive sequence of stars with accurate BVI photometry covering a relatively large (25 x 25 arcmin) region centered on this galaxy. This sequence of standard…

天体物理学 · 物理学 2009-11-07 G. Pietrzynski , W. Gieren , A. Udalski

We present the first four years of BVRI photometry from an on-going survey to annually monitor the photometric behavior of evolved luminous stars in M31 and M33. Photometry was measured for 199 stars at multiple epochs, including 9 classic…

太阳与恒星天体物理 · 物理学 2017-08-09 John C. Martin , Roberta M. Humphreys

The optical UBVRI photometric analysis has been established using SLOAN DIGITAL SKY SURVEY (SDSS database) in order to estimate the astrophysical parameters of poorly studied open star cluster IC 2156. The results of the present study are…

星系天体物理 · 物理学 2017-01-18 A. L. Tadross , Y. H. M. Hendy

We have been doing a photometric and astrometric sample survey programme on Schmidt plates in a few selected directions in the Galaxy with an aim to study galactic stellar populations. In order to calibrate Schmidt plates photometrically,…

We present optical (BVRI) photometric measurements of a sample of 76 common proper motion wide separation main sequence binary pairs. The pairs are composed of a F-, G-, or K-type primary star and an M-type secondary. The sample is selected…

太阳与恒星天体物理 · 物理学 2015-06-22 Ting Li , J. L. Marshall , Sebastien Lepine , Patrick Williams , Joy Chavez

We present a new calibration of optical (UBV, Stromgren, uvby-beta, and Geneva) and near IR (Johnson RIJHK and 2MASS) photometry for B and early A stars derived from Kurucz (1991) Atlas model atmospheres. Our sample of stars consists of 45…

天体物理学 · 物理学 2009-11-10 E. L. Fitzpatrick , D. Massa

We present the first results of a campaign to secure deep UBVRI CCD photometric calibration in all UK Schmidt equatorial fields with galactic latitudes |b| > 50deg. In this paper we provide information on deep BVRI sequences (B<22) in 14 UK…

天体物理学 · 物理学 2015-06-24 B. J. Boyle , T. Shanks , S. M. Croom

We present new multicolour (UBVRcIc) photometric observations of classical symbiotic stars, EG And, Z And, BF Cyg, CH Cyg, CI Cyg, V1329 Cyg, TX CVn, AG Dra, Draco C1, AG Peg and AX Per, carried out between 2007.1 and 2011.9. The aim of…

太阳与恒星天体物理 · 物理学 2015-06-04 A. Skopal , S. Shugarov , M. Vanko , P. Dubovsky , S. P. Peneva , E. Semkov , M. Wolf

Photometric data in the UBV(RI)c system have been acquired for 80 solar analog stars for which we have previously derived highly precise atmospheric parameters Teff, log g, and [Fe/H] using high resolution, high signal-to-noise ratio…

太阳与恒星天体物理 · 物理学 2015-06-04 I. Ramirez , R. Michel , R. Sefako , M. Tucci Maia , W. J. Schuster , F. van Wyk , J. Melendez , L. Casagrande , B. V. Castilho

The beta Cephei stars and slowly pulsating B (SPB) stars are massive main sequence variables. The strength of their pulsational driving strongly depends on the opacity of iron-group elements. As many of those stars naturally occur in young…

太阳与恒星天体物理 · 物理学 2015-05-27 G. Handler
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