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相关论文: Photometric studies of open star clusters Haffner …

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Context. Large-scale surveys across wavelengths, aided by machine learning, have improved the detection of old open clusters in high-extinction Milky Way regions. Aims. We aim to confirm or reject automatically detected open clusters in…

The results of medium-band photometry of 1037 stars in the area of old open cluster NGC 7142 down to V = 20.1 mag in the Vilnius seven-colour system are presented. Photometric results are used to classify in spectral and luminosity classes…

星系天体物理 · 物理学 2013-12-05 V. Straizys , M. Maskoliunas , R. P. Boyle , K. Zdanavicius , J. Zdanavicius , V. Laugalys , A. Kazlauskas

We present here the detailed optical and infra-red photometric analysis of the open star cluster IC 361. On studying the radial density profile, radial extent of the cluster is found to be 8.0 +/- 0.5 arcmin. The basic physical parameters…

太阳与恒星天体物理 · 物理学 2021-06-08 Gireesh C. Joshi

We present $UBVRI$ photometry of 8702 stars in a $0.5 ^\circ\times0.5 ^\circ$ field in the direction of NGC 7142, taken with the Half Degree Imager (HDI) at the WIYN 0.9-meter telescope, to improve knowledge of this cluster's basic…

太阳与恒星天体物理 · 物理学 2020-12-04 Qinghui Sun , Constantine P. Deliyannis , Bruce A. Twarog , Barbara J. Anthony-Twarog , Aaron Steinhauer

To progress in galactic studies based on open clusters, e.g. cluster formation rate or kinematical properties, one needs to improve the number of open clusters observed. However, only half of the 1700 known galactic open clusters have been…

天体物理学 · 物理学 2009-11-11 M. Netopil , H. M. Maitzen , E. Paunzen , A. Claret

We present CCD BV photometry of the intermediate age open cluster Collinder 110, a nearby, scarcely populated, and poorly studied system. There is no literature information on the metallicity, so we tested several possibilities, and found a…

天体物理学 · 物理学 2009-11-07 Angela Bragaglia , Monica Tosi

A (V,V - I)--diagram for the intermediate-age open cluster NGC 7789 has been derived from CCD observations of more than 15,000 stars within ~ 18 arcmin of the cluster center. From the brightest giants and blue stragglers at V ~ 11 to the…

天体物理学 · 物理学 2015-06-24 Munhwan Gim , Don. A. VandenBerg , Peter B. Stetson , James E. Hesser , David R. Zurek

We present CCD BVI photometry of the intermediate age open cluster Pismis 2, covering from the brighter red giants to about 5 magnitudes below the main sequence turn-off. The cluster is heavily reddened and is possibly affected by a…

天体物理学 · 物理学 2009-11-07 L. Di Fabrizio , A. Bragaglia , M. Tosi , G. Marconi

We present photometry in U, B, V, R and I continuum bands and in H$\alpha$ and H$\beta$ emission lines for a sample of 336 circumnuclear star forming regions (CNSFR) located in early type spiral galaxies with different levels of activity in…

星系天体物理 · 物理学 2017-01-04 Mar Álvarez-Álvarez , Angeles I. Díaz , Elena Terlevich , Roberto Terlevich

We present UBVRI photometry of stars in the field of the intermediate-age open cluster NGC 559. By determining the stellar membership probabilities derived through a photometric and kinematic study of the cluster, we identify the 22 most…

星系天体物理 · 物理学 2015-06-17 Yogesh C. Joshi , L. A. Balona , Santosh Joshi , Brijesh Kumar

New photometric material is presented for 6 outer disk supposedly old, Galact ic star clusters: Berkeley 76, Haffner 4, Ruprecht 10, Haffner 7, Haffner 11, and Haffner 15, that are projected against the rich and complex Canis Major overde…

星系天体物理 · 物理学 2015-06-11 Giovanni Carraro , Yuri Beletsky , Gianni Marconi

In this paper we present and analyze new CCD $UBVRI$ photometry down to $V\approx$21 in the region of the young open cluster Trumpler~15, located in the Carina spiral feature. The cluster is rather compact and has a core radius of about…

天体物理学 · 物理学 2009-11-07 Giovanni Carraro

We report on $UBVRI$ CCD photometry of two overlapping fields in the region of the intermediate-age open cluster NGC 2158 down to V=21. By analyzing Colour-Colour (CC) and Colour-Magnitude Diagrams (CMD) we infer a reddening $E_{B-V}=…

天体物理学 · 物理学 2016-08-30 Giovanni Carraro , Leo Girardi , Paola Marigo

We present a detailed photometric and kinematical analysis of poorly studied open cluster IC 1434 using CCD VRI, APASS, and Gaia DR2 database for the first time. BY determining the membership probability of stars, we identified the 238 most…

太阳与恒星天体物理 · 物理学 2021-09-29 Y. H. M. Hendy , D. Bisht

We present UBVRcIc photometric study of three intermediate age open star clusters NGC 381, NGC 2360, and Berkeley 68 (Be 68). We examine the cluster membership of stars using recently released Gaia DR2 proper motions and obtain a total of…

太阳与恒星天体物理 · 物理学 2020-04-07 Jayanand Maurya , Y. C. Joshi

We investigate the old star clusters in the sample of cluster candidates from Froebrich, Scholz & Raftery 2007 -- the FSR list. Based on photometry from the 2-Micron All Sky Survey we generated decontaminated colour-magnitude and…

星系天体物理 · 物理学 2015-05-19 D. Froebrich , S. Schmeja , D. Samuel , P. W. Lucas

We present CCD photometry for the Galactic globular cluster NGC 4833. Our BVI color magnitude diagrams (CMD) extend from above the red giant branch (RGB) tip to several magnitudes below the main sequence turnoff. The principal sequences of…

天体物理学 · 物理学 2009-10-31 Jason Melbourne , Ata Sarajedini , Andrew Layden , Donald H. Martins

In this paper we present UBVRI CCD photometry in the region of two young open star clusters Basel 4 and NGC 7067 for the first time. Our sample consists of ~ 4000 stars down to V ~ 21 mag. Stellar surface density profile indicates that…

天体物理学 · 物理学 2009-11-10 R. K. S. Yadav , Ram Sagar

Photometric CCD {\it UBVI}$_C$ photometry obtained for 4860 stars surrounding the embedded southern cluster SAI~113 (Skiff~8) is used to examine the reddening in the field and derive the distance to the cluster and nearby van~Genderen~1.…

星系天体物理 · 物理学 2017-03-22 Giovanni Carraro , David Turner , Daniel Majaess , Gustavo Baume , Roberto Gamen , Jose Molina Lera

We present $UBVI_C$ CCD photometry of the young open cluster Be 59 with the aim to study the star formation scenario in the cluster. The radial extent of the cluster is found to be $\sim$ 10 arcmin (2.9 pc). The interstellar extinction in…

天体物理学 · 物理学 2009-11-13 A. K. Pandey , Saurabh Sharma , K. Ogura , D. K. Ojha , W. P. Chen , B. C. Bhatt , S. K. Ghosh