English
Related papers

Related papers: The open cluster King~1 in the second quadrant

200 papers

Aims. We aim to investigate the stellar population properties, ages, and metal content of the globular clusters (GCs) in NGC 3311, the central galaxy of the Hydra I cluster, to better constrain its evolution history. Methods. We used…

We utilize Gaia DR3 data to report the discovery of a new star cluster, Nasser 1, located 32 arcmin from Czernik 38 at coordinates $\alpha= 282.11 \pm 0.05$ and $\delta= 4.56 \pm 0.05$. Using a variable membership probability threshold…

Astrophysics of Galaxies · Physics 2026-01-15 Nasser M. Ahmed

Spectra from MDM Observatory are used to assess Lick/IDS feature strength gradients inside the half-light radius of the compact Local Group elliptical galaxy M32. All but a few (of 24 measured) indices show a statistically significant…

Astrophysics · Physics 2009-11-10 Guy Worthey

Precision uvbyCa Hbeta photometry of the metal-deficient, old open cluster, NGC 2506, is presented. The survey covers an area 20 by 20 arcminutes, and extends to V~18 for b-y and Hbeta and to V~17.0 for c_1 and hk. For V < 16.0, photometric…

Solar and Stellar Astrophysics · Physics 2016-12-07 B. J. Anthony-Twarog , C. P. Deliyannis , B. A. Twarog

HIRES on the Keck I telescope has been used to measure the first radial velocities for stars belonging to eleven, heavily-reddened globular clusters in the direction of the inner Galaxy. The question of kinematic substructuring among the…

Astrophysics · Physics 2011-03-28 Patrick Cote

M 39 is a nearby young open cluster hardly studied in the last decades. No giant is known among its members and its chemical composition has never been studied. In order to investigate it we performed high-resolution spectroscopy of 20…

Astrophysics of Galaxies · Physics 2023-12-15 J. Alonso-Santiago , A. Frasca , G. Catanzaro , A. Bragaglia , L. Magrini , A. Vallenari , E. Carretta , S. Lucatello

We present the high resolution (R $\approx$ 60000), high signal-to-noise (S/N $\simeq$ 120) spectroscopic analysis of 12 red giant members of the Galactic open cluster NGC 6940. We applied Yonsei-Yale isochrones to the color-magnitude…

Solar and Stellar Astrophysics · Physics 2019-03-12 G. Böcek Topcu , M. Afşar , C. Sneden

In this paper we have compiled two new open cluster catalogues. In the first one, there are 119 objects with ages, distances and metallicities available, while in the second one, 144 objects have both absolute proper motion and radial…

Astrophysics · Physics 2009-11-07 L. Chen , J. L. Hou , J. J. Wang

We used a proper combination of high-resolution HST observations and wide-field ground based data to derive the radial star density profile of 26 Galactic globular clusters from resolved star counts (which can be all freely downloaded…

Astrophysics of Galaxies · Physics 2013-08-28 P. Miocchi , B. Lanzoni , F. R. Ferraro , E. Dalessandro , E. Vesperini , M. Pasquato , G. Beccari , C. Pallanca , N. Sanna

We present precision radial velocities and stellar population parameters for 77 star clusters in the Local Group galaxy M33. Our GTC and WHT observations sample both young, massive clusters and known/candidate globular clusters, spanning…

Astrophysics of Galaxies · Physics 2015-04-24 Michael A. Beasley , Izaskun San Roman , Carme Gallart , Ata Sarajedini , Antonio Aparicio

We present internal velocity dispersions and precise radial velocities for 200 globular clusters (GCs) in M31 that are derived using new high-resolution spectra from MMT/Hectochelle. Of these, 163 also have King model structural parameters…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 Jay Strader , Nelson Caldwell , Anil Seth

CCD $BVI$ photometry is presented for 8 previously unstudied star clusters located in the First and Fourth Galactic Quadrants: AL~1, BH 150, NGC 5764, Lynga~9, Czernik~37, BH 261, Berkeley~80 and King~25. Color magnitude diagrams of the…

Astrophysics · Physics 2009-11-13 Giovanni Carraro , Kenneth A. Janes , Jason D. Eastman

In the context of a project aimed at characterizing the properties of star clusters in the Galactic bulge, here we present the determination of the internal kinematics and structure of the massive globular cluster NGC 6569. The kinematics…

We present deep optical and near-infrared imaging of the rich cluster A2218 at z=0.17. Our optical imaging comes from new multicolour Hubble Space Telescope WFPC2 observations in the F450W (B), F606W (V) and F814W (I) passbands. These…

Astrophysics · Physics 2015-06-24 Ian Smail , Harald Kuntschner , T. Kodama , G. P. Smith , C. Packham , A. S. Fruchter , R. N. Hook

We derive fundamental parameters for the old, rich open cluster NGC 1245 using BVI photometry from the MDM 1.3m and 2.4m telescopes. Based on detailed isochrone fitting, we find NGC 1245 has a slightly sub-solar metallicity, [Fe/H]=-0.05 +-…

We present deep CCD photometry of the very rich, intermediate aged (similar to the Hyades) open star cluster NGC 2099 (M37). The V, B-V color-magnitude diagram (CMD) for the cluster shows an extremely well populated and very tightly…

The Hydra I cluster offers an excellent opportunity to study and compare the relic old stellar populations in the core of its two brightest galaxies. In addition, the differing kinematics of the two galaxies allows a test of the local…

Astrophysics of Galaxies · Physics 2023-05-17 Ilaria Lonoce , Wendy Freedman , Anja Feldmeier-Krause

We present the analysis of an eccentric, partially eclipsing long-period ($P=19.23$ d) binary system KIC 9777062 that contains main sequence stars near the turnoff of the intermediate age open cluster NGC 6811. The primary is a metal-lined…

This study is an investigation of the stellar density profile of the Galactic disc in the Anticentre direction. We select over 40,000 early A stars from IPHAS photometry in the Galactic longitude range 160 < l < 200 close to the equatorial…

We have obtained medium-low resolution spectroscopy and BVI CCD imaging of Berkeley 32, an old open cluster which lies in the anticentre direction. From the radial velocities of 48 stars in the cluster direction we found that 31 of them, in…

Astrophysics · Physics 2009-11-11 V. D'Orazi , A. Bragaglia , M. Tosi , L. Di Fabrizio , E. V. Held
‹ Prev 1 3 4 5 6 7 10 Next ›