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相关论文: The embedded cluster DBSB48 in the nebula Hoffleit…

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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

Trumpler 5 is a moderately old, dust-obscured metal-poor open cluster. In this study, high-resolution near-infrared spectroscopic data of seven giant stars from the Trumpler 5 cluster were analyzed to derive chemical abundances for 20…

太阳与恒星天体物理 · 物理学 2025-07-09 S. Özdemir , M. Afşar , C. Sneden , D. A. VandenBerg , P. A. Denissenkov , A. P. Milone , Z. Bozkurt , H. Oh , K. Sokal , G. N. Mace , D. T. Jaffe

As part of a long term programme, we analyse the evolutionary status and properties of the old and populous open cluster Trumpler 5 (Tr 5), located in the Galactic anticentre direction, almost on the Galactic plane. Tr 5 was observed with…

太阳与恒星天体物理 · 物理学 2015-06-23 P. Donati , G. Cocozza , A. Bragaglia , E. Pancino , T. Cantat-Gaudin , R. Carrera , M. Tosi

Deep CCD photometry in the uvby-Hbeta intermediate-band system is presented for the cluster NGC 2548 (M 48). A complete membership analysis based on astrometric and photometric criteria is applied. The photometric analysis of a selected…

天体物理学 · 物理学 2015-12-24 L. Balaguer-Nunez , C. Jordi , D. Galadi-Enriquez

Context: Trumpler 23 is a moderately populated, intermediate-age open cluster within the solar circle at a Rgc ~6 kpc. It is in a crowded field very close to the Galactic plane and the color-magnitude diagram shows significant field…

Using the highest-resolution X-ray observation of the Trumpler 15 star cluster taken by the Chandra X-ray Observatory, we estimate the total size of its stellar population by comparing the X-ray luminosity function of the detected sources…

We present a study of the mass accretion rates of pre-Main Sequence (PMS) stars in the cluster Trumpler 14 (Tr14) in the Carina Nebula. Using optical multi-band photometry we were able to identify 356 PMS stars showing H-alpha excess…

太阳与恒星天体物理 · 物理学 2015-06-22 G. Beccari , G. DeMarchi , N. Panagia , E. Valenti , G. Carraro , M. Romaniello , M. Zoccali , C. Weidner

We present results from Johnson $UBV$, Kron-Cousins $RI$ and Washington $CT_1T_2$ photometries for seven van den Bergh-Hagen (vdBH) open clusters, namely, vdBH\,1, 10, 31, 72, 87, 92, and 118. The high-quality, multi-band photometric data…

星系天体物理 · 物理学 2016-09-21 Andrés E. Piatti

The results of the complex study of galactic open cluster Trumpler 2 are presented. In order to obtain the proper motions the positions of 2600 stars up to the limit magnitude B ~ 16.25 mag in the area 80x80 arcmin around the cluster were…

天体物理学 · 物理学 2009-11-11 V. N. Frolov , J. K. Ananjevskaja , E. G. Jilinski , D. L. Gorshanov

UBVRI CCD photometry of a $2.^{\prime}1 \times 3.^{\prime}3$ field centered on the young open cluster Haffner~18 is presented and discussed. Spectroscopic classification of seven stars is also provided. 44 clusters members are identified,…

天体物理学 · 物理学 2009-10-30 Ulisse Munari , Giovanni Carraro , Roberto Barbon

We present deep UBVI photometry for Trumpler 20, a rich, intermediate-age open cluster located at l=301.47, b=+2.22 (RA=12:39:34, DEC=-60:37:00, J2000.0) in the fourth Galactic quadrant. In spite of its interesting properties, this cluster…

星系天体物理 · 物理学 2015-05-19 Giovanni Carraro , Edgardo Costa , Javier Ahumada

With an apparent cluster diameter of 1.5{\deg} and an age of ~4 Myr, Trumpler 37 is an ideal target for photometric monitoring of young stars as well as for the search of planetary transits, eclipsing binaries and other sources of…

We present a detailed near-infrared study of an embedded cluster located in the hub of the giant molecular cloud G148.24+00.41 of mass $\sim$10$^5$ $M_\odot$, with the TANSPEC instrument mounted on the 3.6 m Devasthal Optical Telescope. The…

星系天体物理 · 物理学 2024-08-26 Vineet Rawat , M. R. Samal , D. K. Ojha , Brajesh Kumar , Saurabh Sharma , J. Jose , Ram Sagar , R. K. Yadav

We derive photometric, structural and dynamical evolution-related parameters of five as yet unstudied low-contrast open clusters located in the third quadrant using 2MASS data. The target clusters are Czernik 31, Czernik 32, Haffner 9,…

天体物理学 · 物理学 2007-05-23 E. Bica C. Bonatto

We have carried out deep (V$\sim$21 mag) \ubvri photometric study of the star cluster Stock 18. These along with archival Infrared data have been used to derive the basic cluster parameters and also to study the star formation processes in…

太阳与恒星天体物理 · 物理学 2015-05-30 Himali Bhatt , Ram Sagar , J. C. Pandey

NGC 6819 is a richly populated, older open cluster situated within the Kepler field. A CCD survey of the cluster on the uvbyCaHbeta system, coupled with proper-motion membership, has been used to isolate 382 highly probable, single-star…

太阳与恒星天体物理 · 物理学 2015-06-22 B. J. Anthony-Twarog , C. P. Deliyannis , B. A. Twarog

In this paper we present and analyze new CCD $UBVRI$ photometry down to $V \approx$ 21 in the region of the young open cluster Collinder 232, located in the Carina spiral arm, and discuss its relationship to Trumpler 14 and Trumpler 16, the…

天体物理学 · 物理学 2009-11-10 Giovanni Carraro , Martino Romaniello , Paolo Ventura , Ferdinando Patat

We present the results of an infrared photometric survey performed with NICS@TNG in the nearby starburst galaxy NGC 4214. We derived accurate integrated JK magnitudes of 10 young massive clusters and compared them with the already available…

宇宙学与河外天体物理 · 物理学 2015-06-15 A. Sollima , R. G. Gratton , E. Carretta , A. Bragaglia , S. Lucatello

In order to investigate the Galactic-scale environmental effects on the evolution of protoplanetary disks, we explored the near-infrared (NIR) disk fraction of the Quartet cluster, which is a young cluster in the innermost Galactic disk at…

太阳与恒星天体物理 · 物理学 2016-02-17 Chikako Yasui , Naoto Kobayashi , Satoshi Hamano , Sohei Kondo , Natsuko Izumi , Masao Saito , Alan T. Tokunaga

A high number of embedded clusters is found in the Galaxy. Depending on the formation scenario, most of them can evolve to unbounded groups that are dissolved within a few tens of Myr. A systematic study of young stellar clusters showing…

星系天体物理 · 物理学 2015-06-11 T. Santos-Silva , J. Gregorio-Hetem
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