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相关论文: The Young Open Cluster NGC 2129

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Images and spectra of the open cluster NGC 3105 have been obtained with GMOS on Gemini South. The (i', g'-i') color-magnitude diagram (CMD) constructed from these data extends from the brightest cluster members to g'~23. This is 4 - 5 mag…

星系天体物理 · 物理学 2017-03-22 T. J. Davidge

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

The young cluster NGC 6231 (stellar ages ~2-7 Myr) is observed shortly after star-formation activity has ceased. Using the catalog of 2148 probable cluster members obtained from Chandra, VVV, and optical surveys (Paper I), we examine the…

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

Precision uvbyCaHbeta photometry of the nearby old open cluster, NGC 752, is presented. The mosaic of CCD fields covers an area ~42' on a side with internal precision at the 0.005 to 0.010 mag level for the majority of stars down to V~15.…

太阳与恒星天体物理 · 物理学 2015-10-14 B. A. Twarog , B. J. Anthony-Twarog , C. P. Deliyannis , D. T. Thomas

Multi-wavelength CCD photometry over 21 years has been used to produce deep color-magnitude diagrams together with light curves for the variables in the Galactic globular cluster NGC 5824. Twenty-one new cluster RR Lyrae stars are…

We present CCD uvby-beta photometry for stars in the nuclei of the young double cluster h and chi Persei. We find that the reddening is highly variable through the h Persei nucleus, increasing from west to east, with values ranging from…

天体物理学 · 物理学 2009-11-07 G. Capilla , J. Fabregat

We present a method for finding clusters of young stars in M31 using broadband WFPC2 data from the HST data archive. Applying our identification method to 13 WFPC2 fields, covering an area of ~60 arcmin^2, has revealed 79 new candidate…

天体物理学 · 物理学 2009-11-06 Benjamin F. Williams , Paul W. Hodge

We present CCD UBVI photometry of the intermediate old open cluster NGC2660, covering from the red giants region to about seven magnitudes below the main sequence turn-off. Using the synthetic Colour - Magnitude Diagram method, we estimate…

天体物理学 · 物理学 2009-10-31 S. Sandrelli , A. Bragaglia , M. Tosi , G. Marconi

We use CCD and photoelectric photometry with Stromgren filters along with medium resolution spectra to investigate NGC 6520, an open cluster very nearly in the direction of the galactic center. We find an age of 60 Myr, a distance of 2 kpc,…

太阳与恒星天体物理 · 物理学 2015-06-17 Andrew P. Odell

We present UBVRI photometry for the old open cluster NGC 6253. From comparison of the observed colour-magnitude diagrams with simulations based on stellar evolutionary models we derive in a self consistent way reddening, distance, and age…

天体物理学 · 物理学 2015-06-24 A. Bragaglia , G. Tessicini , M. Tosi , G. Marconi , U. Munari

We have carried out WFPC2 V- and I-band imaging of the young LMC cluster NGC 2157. Construction of a color-magnitude diagram and isochrone fitting yields an age of tau = 100 000 000 yrs, a reddening E(B-V) = 0.1 and a distance modulus of…

天体物理学 · 物理学 2007-05-23 Philippe Fischer , Carlton Pryor , Stephen Murray , Mario Mateo , Tom Richtler

We present the broad band UBVI CCD photometric investigations in the region of the two open clusters Haffner 11 and Czernik 31. The radii of the clusters are determined as 3.5 arcmin and 3.0 arcmin for Haffner 11 and Czernik 31…

星系天体物理 · 物理学 2015-06-15 D. Bisht , R. K. S. Yadav , A. K. Durgapal

We present the first $BVI$ CCD photometry to $V=22.0$ of 4 fields centered on the region of the southern Galactic star clusters Ruprecht~61, Czernik~32, NGC 2225 and NGC 2262 and of 4 displaced control fields. These clusters were never…

天体物理学 · 物理学 2009-11-13 G. Carraro , G. Baume , R. Vazquez , A. Moitinho , D. Geisler

We report the results of a time-series CCD photometric survey of variable stars in the field of the open cluster NGC 2126. In about one square degree field covering the cluster, a total number of 21 variable candidates are detected during…

太阳与恒星天体物理 · 物理学 2009-07-22 Shun-Fang Liu , Zhen-Yu Wu , Xiao-Bin Zhang , Jiang-Hua Wu , Jun Ma , Zhao-Ji Jiang , Jian-Sheng Chen , Xu Zhou

We present the results of a deep, wide-field CCD survey for the open cluster NGC~3532. Our new $BV(RI)_{c}$ photometry effectively covers a one square degree area and reaches an unprecedented depth of $V\sim21$ to reveal that NGC~3532 is a…

太阳与恒星天体物理 · 物理学 2015-05-27 James L. Clem , Arlo U. Landolt , D. W. Hoard , Stefanie Wachter

We have investigated the area of two NGC entries, NGC 1817 and NGC 1807, with deep CCD photometry in the uvby-Hbeta intermediate-band system. The photometric analysis of a selected sample of stars of the open cluster NGC 1817 yields a…

天体物理学 · 物理学 2009-11-10 L. Balaguer-Nunez , C. Jordi , D. Galadi-Enriquez , E. Masana

We present new multiband photometry for the Galactic globular cluster IC 4499 extending well past the main sequence turn-off in the U, B, V, R, I, and DDO51 bands. This photometry is used to determine that IC4499 has an age of 12 pm 1 Gyr…

We present BV CCD photometry for the open clusters Czernik 24 and Czernik 27. These clusters have never been studied before, and we provide, for the first time, the cluster parameters; reddening, distance, metallicity and age. Czernik 24 is…

We present deep wide-field optical CCD photometry and mid-infrared Spitzer/IRAC and MIPS 24micron data for about 100,000 stars in the young open cluster IC 1805. The members of IC 1805 were selected from their location in the various…

太阳与恒星天体物理 · 物理学 2020-12-09 Hwankyung Sung , Michael S. Bessell , Moo-Young Chun , Jonghyuk Yi , Y. Naze , Beomdu Lim , R. Karimov , G. Rauw , Byeong-Gon Park , Hyeonoh Hur