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相关论文: The stellar content of the young open cluster Trum…

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We present a photometric and spectroscopic study of the poorly investigated open cluster Trumpler~3. Basic parameters such as the age of $70\pm10$ Myr, the color excess $E(B-V)=0.30\pm0.02$ mag, the distance of $0.69\pm0.03$ kpc and the…

星系天体物理 · 物理学 2015-05-18 G. Maciejewski , L. Bukowiecki

We present an investigation of the open cluster Trumpler 2 using Gaia DR3 photometric, astrometric and spectroscopic data. 92 stars were identified as likely members of the cluster, with membership probabilities greater than 0.5. The mean…

星系天体物理 · 物理学 2023-04-28 S. Tasdemir , T. Yontan

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

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

We present results of the first extensive and deep CCD photometric survey carried out in the field of the open cluster Trumpler 27, an object in the constellation of Sagittarius not far from the Galaxy center. We look for young stars clumps…

星系天体物理 · 物理学 2015-06-03 Gabriel Perren , Rubén Vázquez , Giovanni Carraro

Aims. The main goal of this work is to date young open clusters using $\delta$ Sct stars. Seismic indices such as the large separation and the frequency at maximum power can help to constrain the models to better characterise the stars. We…

太阳与恒星天体物理 · 物理学 2023-07-19 D. Pamos Ortega , G. M. Mirouh , A. García Hernández , J. C. Suárez Yanes , S. Barceló Forteza

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…

Determination of stellar age is a crucial task in astrophysics research. Different methods are nowadays used either model dependent or based on calibrated empirical relations. The most reliable results are generally obtained when different…

太阳与恒星天体物理 · 物理学 2021-01-27 Sergio Messina

It is currently widely accepted that open star clusters and stellar associations result from the evolution of embedded star clusters. Parameters such star formation efficiency, time-scale of gas removal and velocity dispersion can be…

星系天体物理 · 物理学 2015-06-03 T. A. Saurin , E. Bica , C. Bonatto

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

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

This paper reports results from our long-term $BV(RI)_{c}$ photometric CCD observations of eight pre-main-sequence stars collected from June 2008 to October 2022. These stars are located in the young open cluster Trumpler 37, in the field…

太阳与恒星天体物理 · 物理学 2023-07-26 Sunay Ibryamov , Gabriela Zidarova , Evgeni Semkov , Stoyanka Peneva

Identifying and characterizing young populations of star-forming regions is crucial to unravel their properties. In this regard, Gaia-DR3 data and machine learning tools are very useful for studying large star-forming complexes. In this…

星系天体物理 · 物理学 2023-05-03 Swagat R. Das , Saumya Gupta , Prem Prakash , Manash Samal , Jessy Jose

We analyse multi-wavelength observations of 32 young star clusters and associations in M33 with known oxygen abundance (8 < 12 + log(O/H) < 8.7), using ultraviolet (UV), optical, mid-infrared (MIR), CO (1-0) and 21-cm line (HI)…

宇宙学与河外天体物理 · 物理学 2015-05-19 M. Grossi , E. Corbelli , C. Giovanardi , L. Magrini

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…

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

We present new UBVI_C CCD photometry of the young open clusters Trumpler 14 (Tr 14) and Trumpler 16 (Tr 16) in the eta Carina nebula. We also identify the optical counterpart of Chandra X-ray sources and Two Micron All Sky Survey point…

太阳与恒星天体物理 · 物理学 2015-06-03 Hyeonoh Hur , Hwankyung Sung , Michael S. Bessell

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

Stars in open clusters are powerful probes of the intervening Galactic magnetic field, via background starlight polarimetry, because they provide constraints on the magnetic field distances. We use 2MASS photometric data for a sample of 31…

太阳与恒星天体物理 · 物理学 2015-10-14 Sadia Hoq , Dan Clemens
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