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Related papers: The anomalous Galactic globular cluster NGC 2808

200 papers

We perform a detailed study of the Globular Cluster (GC) system in the galaxy NGC5866 based on F435W, F555W, and F625W (~ B, V, and R) HST Advanced Camera for Surveys images. Adopting color, size and shape selection criteria, the final list…

Astrophysics · Physics 2015-05-13 Cantiello , Michele , Blakeslee , John P. , Raimondo , Gabriella

We present new VI photometry for the halo globular cluster M30 (NGC 7099), and compute luminosity functions (LFs) in both bands for samples of about 15,000 hydrogen-burning stars from near the tip of the red giant branch (RGB) to over four…

We report CCD photometric observations of the globular cluster NGC 5897, in the Johnson system filters B, V , R, and I. With the values for these magnitudes we obtain various colour indices and produce several colour-magnitude diagrams. We…

Solar and Stellar Astrophysics · Physics 2023-11-14 A. Ruelas-Mayorga , L. J. Sánchez , E. Macías-Estrada , A. Nigoche-Netro

We present radial and rotation (v sini) velocity measurements, from UVES+VLT high resolution spectra of 61 stars in the blue horizontal branches (HB) of the Galactic globular clusters NGC 1904 (M79), NGC 2808, NGC 6093 (M80), and NGC 7078…

Astrophysics · Physics 2009-11-10 Alejandra Recio-Blanco , Giampaolo Piotto , Antonio Aparicio , Alvio Renzini

We present ultraviolet photometry for globular clusters (GCs) in M31 from 15 square deg of imaging using the Galaxy Evolution Explorer (GALEX). We detect 200 and 94 GCs with certainty in the near-ultraviolet (NUV; 1750 - 2750 Angstroms) and…

We studied the color distribution of the main sequence of the Globular Cluster NGC 2808, based on new deep HST-WFPC2 photometry of a field in the uncrowded outskirts of the cluster. The color distribution of main sequence stars is wider…

Astrophysics · Physics 2008-11-26 F. D'Antona , M. Bellazzini , V. Caloi , F. Fusi Pecci , S. Galleti , R. T. Rood

The large and diffuse galaxies NGC1052-DF2 and NGC1052-DF4 have been found to have very low dark matter content and a population of luminous globular clusters. Accurate distance measurements are key to interpreting these observations.…

We present the first results from our HST Brightest Cluster Galaxy (BCG) survey of seven central supergiant cluster galaxies and their globular cluster (GC) systems. We measure a total of 48000 GCs in all seven galaxies, representing the…

We present a CCD investigation of the galactic globular M5 aimed to increase the statistical relevance of the available sample of evolving bright stars. Previous investigations, limited to the outer cluster region, have been extended toward…

Astrophysics · Physics 2009-10-22 E. Brocato , V. Castellani , V. Ripepi

Galactic globular clusters (GCs) are now known to host multiple populations displaying particular abundance variations. The different populations within a GC can be well distinguished following their position in the pseudo two-colors…

Solar and Stellar Astrophysics · Physics 2019-10-16 M. Latour , T. -O. Husser , B. Giesers , S. Kamann , F. Goettgens , S. Dreizler , J. Brinchmann , N. Bastian , M. Wendt , P. M. Weilbacher , N. S. Molinski

We have used WFPC2 to construct B, V color-magnitude diagrams of four metal-rich globular clusters, NGC 104 (47 Tuc), NGC 5927, NGC 6388, and NGC 6441. All four clusters have well populated red horizontal branches (RHB), as expected for…

We have obtained HST/STIS far- and near-UV photometry of globular clusters in four fields in the gE galaxy M87. To a limit of m(FUV) = 25 we detect a total of 66 globular clusters (GCs) in common with the deep HST optical-band study of…

Deep BV photometry for a large field covering the outer-halo globular cluster NGC 6229 is presented. For the first time, a colour-magnitude diagram (CMD) reaching below the main sequence turnoff has been obtained for this cluster. Previous…

Context. Extratidal stars are stellar bodies that end up outside the tidal radius of a cluster as a result of internal processes or external forces acting upon it. The presence and spatial distribution of these stars can give us insights…

NGC 1851 is an intriguing Galactic globular cluster, with multiple stellar evolutionary sequences, light and heavy element abundance variations and indications of a surrounding stellar halo. We present the first results of a spectroscopic…

Solar and Stellar Astrophysics · Physics 2015-08-26 Colin A. Navin , Sarah L. Martell , Daniel B. Zucker

We present new BVI photometry for the halo globular cluster M5, and examine the B- and I-band luminosity functions (LFs), based on over 20,000 stars. We do not see evidence in the LF of a ``subgiant excess'' or of a discrepancy in the…

Astrophysics · Physics 2009-10-28 Eric L. Sandquist , Michael Bolte , Peter B. Stetson

We use images acquired with the Hubble Space Telescope Wide Field Camera 3 and new models to probe the Horizontal Branch (HB) population of the We use images acquired with the Hubble Space Telescope Wide Field Camera 3 and new models to…

Solar and Stellar Astrophysics · Physics 2015-07-22 M. Di Criscienzo , M. Tailo , A. P. Milone , F. D'Antona , P. Ventura , A. Dotter , E. Brocato

We report results from Hubble Space Telescope WFPC2 imaging of the field of the luminous, bursting X-ray source in the globular cluster NGC 6441. Although the X-ray position is known to a precision of a few arcseconds, this source is only…

Astrophysics · Physics 2009-10-30 Eric W. Deutsch , Scott F. Anderson , Bruce Margon , Ronald A. Downes

NGC 2419 is a peculiar Galactic globular cluster in terms of size/luminosity, and chemical abundance anomalies. Here, we present Str\"omgren $uvby$ photometry of the cluster. Using the gravity- and metallicity-sensitive $c_1$ and $m_1$…

Astrophysics of Galaxies · Physics 2015-10-12 Matthias J. Frank , Andreas Koch , Sofia Feltzing , Nikolay Kacharov , Mark I. Wilkinson , Mike Irwin

We present $BVI$ photometry for about 16000 stars from a 220 arcmin$^{2}$ field centered 8 arcmin east of the center of 47 Tuc. We have identified eight likely blue stragglers located in the outer parts of the cluster. Four of these objects…

Astrophysics · Physics 2007-05-23 J. Kaluzny , A. Wysocka , K. Z. Stanek , W. Krzeminski
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