中文
相关论文

相关论文: Photometric and spectroscopic study of the interme…

200 篇论文

We present a $BVI$ photometric and astrometric catalogue of the open cluster NGC 3960, down to limiting magnitude $V\sim22$, obtained from observations taken with the Wide Field Imager camera at the MPG/ESO 2.2 m Telescope at La Silla. The…

天体物理学 · 物理学 2009-11-10 L. Prisinzano , G. Micela , S. Sciortino , F. Favata

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 present CCD UBVI photometry of the nearby, intermediate age open cluster NGC 6939. Using the synthetic Colour - Magnitude Diagrams technique we estimate the following parameters: age between 1.3 and 1.0 Gyr (depending on whether or not…

天体物理学 · 物理学 2009-11-10 Gloria Andreuzzi , Angela Bragaglia , Monica Tosi , Gianni Marconi

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 and discuss broad band CCD $UBV(I)_C$ photometry and low resolution spectroscopy for stars in the region of the open cluster NGC 6996, located in the North America Nebula. The new data allow us to tightly constrain the basic…

天体物理学 · 物理学 2009-11-10 Sandro Villanova , Gustavo Baume , Giovanni Carraro , Anna Geminale

We report on $BVI$ CCD photometry of a field centered on the region of the intermediate-age open cluster NGC 2112 down to V=21. Due to the smaller field coverage, we are able to limit the effect of field star contamination which hampered in…

天体物理学 · 物理学 2009-11-07 Giovanni Carraro , Roberto Barbon , Carla S. Boschetti

The B,V CCD photometry of 916 stars in the field of the high galactic latitude intermediate age open cluster NGC 1245 is presented. The cluster parameters were estimated with the help of V vs (B-V) colour-magnitude diagram (CMD). After…

天体物理学 · 物理学 2007-05-23 Annapurni Subramaniam

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

We derive accurate parameters related to the CMD, structure and dynamical state of M52 and NGC3960, whose fields are affected by differential reddening. Compared to open clusters in different dynamical states studied with similar methods,…

天体物理学 · 物理学 2009-11-11 C. Bonatto , E. Bica

CCD photometry on the uvbyCaHbeta system is presented for the open cluster, NGC 3680. Restricting the data to probable cluster members using the CMD and the photometric indices alone defines a sample of 34 stars at the cluster turnoff that…

天体物理学 · 物理学 2009-11-10 B. J. Anthony-Twarog , B. A. Twarog

Fundamental astrophysical parameters have been derived for 20 open clusters (O\!Cs) using CCD~$U\!BV\!(RI)_C$ photometric data observed with the 84~cm telescope at the San Pedro M\'artir National Astronomical Observatory, M\'exico. The…

星系天体物理 · 物理学 2015-06-22 Inci Akkaya Oralhan , Yüksel Karataş , William J. Schuster , Raúl Michel , Carlos Chavarría

The fundamentals of estimating essential stellar parameters of an open cluster-NGC 2360 and globular clusters-NGC 5272 are presented extensively in this work. Here, the evaluation of stellar parameters, by manually fitting the appropriate…

星系天体物理 · 物理学 2022-11-09 Kanwar Preet Kaur , Pankaj S. Joshi

We present a photometric analysis of the star clusters Lindsay 1, Kron 3, NGC339, NGC416, Lindsay 38, and NGC419 in the Small Magellanic Cloud (SMC), observed with the Hubble Space Telescope Advanced Camera for Surveys (ACS) in the F555W…

We present UBV CCD observations obtained in the field of the northern open cluster NGC 1220, for which little information is available. We provide also BV CCD photometry of a field 5$^{\prime}$ northward of NGC 1220 to take into account…

天体物理学 · 物理学 2009-11-07 S. Ortolani , G. Carraro , S. Covino , E. Bica , B. Barbuy

We analyzed HST/WFPC2 colour-magnitude diagrams (CMDs) of 15 populous Large Magellanic Cloud (LMC) stellar clusters with ages between ~ 0.3 Gyr and ~ 3 Gyr. These (V, B-V) CMDs are photometrically homogeneous and typically reach V \~ 22.…

天体物理学 · 物理学 2009-11-11 L. O. Kerber , B. X. Santiago , E. Brocato

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

CCD photometry on the intermediate-band uvbyCa H beta system is presented for the anticenter, intermediate-age open cluster, Melotte 71. Restricting the data to probable single members of the cluster using the color-magnitude diagram and…

天体物理学 · 物理学 2008-11-26 B. A. Twarog , S. Corder , B. J. Anthony-Twarog

We present and discuss new photometric data obtained with an IR camera in the J and K pass-bands for the intermediate age open clusters IC 166 (936 stars in total) and NGC 7789 (1030 stars in total). Ic 166 is a poorly studied open cluster…

天体物理学 · 物理学 2007-05-23 Antonella Vallenari , Giovanni Carraro , Andrea Richichi

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

We present colour-magnitude diagrams (CMDs) for a sample of seven young massive clusters in the galaxies NGC 1313, NGC 1569, NGC 1705, NGC 5236 and NGC 7793. The clusters have ages in the range 5-50 million years and masses of 10^5 -10^6…

星系天体物理 · 物理学 2015-05-28 S. S. Larsen , S. E. de Mink , J. J. Eldridge , N. Langer , N. Bastian , A. Seth , L. J. Smith , J. Brodie , Y. N. Efremov
‹ 上一页 1 2 3 10 下一页 ›