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相关论文: A Homogenous Set of Globular Cluster Relative Dist…

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We build differential-reddening maps for 66 Galactic globular clusters (GCs) with archival HST WFC/ACS F606W and F814W photometry. Because of the different GC sizes (characterised by the half-light radius $R_h$) and distances to the Sun,…

星系天体物理 · 物理学 2015-06-16 Charles Bonatto , Fabíola Campos , Kepler S. Oliveira

Grids of zero-age horizontal branch (ZAHB) models are presented, along with a suitable interpolation code, for -2.5 <= [Fe/H] <= -0.5, in steps of 0.2 dex, assuming Y = 0.25 and 0.29, [O/Fe] = +0.4 and +0.6, and [m/Fe] = 0.4 for all of the…

星系天体物理 · 物理学 2023-11-14 Don A. VandenBerg

We report new HST/WFPC2 photometry for 10 globular clusters (GC) in M31 observed in F5555W(V) and F814W(I). Additionally we have reanalyzed HST archival data of comparable quality for 2 more GCs. Extraordinary care is taken to account for…

天体物理学 · 物理学 2009-11-10 R. M. Rich , C. E. Corsi , C. Cacciari , L. Federici , F. Fusi Pecci , S. G. Djorgovski

The presence of differential reddening in the direction of Galactic globular clusters (GCs) has proven to be a serious limitation in the traditional colour-magnitude diagram (CMD) analysis. Here, we estimate local reddening variations in…

By adopting the same approach outlined in De Santis & Cassisi (1999), we evaluate the absolute bolometric magnitude of the Zero Age Horizontal Branch (ZAHB) at the level of the RR Lyrae variable instability strip in selected galactic…

天体物理学 · 物理学 2009-11-06 S. Cassisi , R. De Santis , A. M. Piersimoni

Ages have been derived for 55 globular clusters (GCs) from overlays of isochrones onto the turnoff photometry, assuming distances based on fits of zero-age horizontal branch (ZAHB) models to the lower bound of the observed distributions of…

星系天体物理 · 物理学 2013-10-14 Don A. Vandenberg , Karsten Brogaard , Ryan Leaman , Luca Casagrande

We use the Stetson, HST, and Gaia DR3 data sets for 22 Galactic globular clusters to select their members and fit their CMDs with isochrones from DSED and BaSTI for $[\alpha/$Fe$]=+0.4$ and an adopted helium mass fraction $Y$. As a result,…

星系天体物理 · 物理学 2026-05-28 G. A. Gontcharov , O. S. Ryutina , C. J. Bonatto , S. S. Savchenko , S. V. Troitsky

We present precise and deep optical photometry of the globular M92. Data were collected in three different photometric systems: Sloan Digital Sky Survey (g',r',i',z'; MegaCam@CFHT), Johnson-Kron-Cousins (B, V, I; various ground-based…

We present CCD photometry for the Galactic globular cluster NGC 4833. Our BVI color magnitude diagrams (CMD) extend from above the red giant branch (RGB) tip to several magnitudes below the main sequence turnoff. The principal sequences of…

天体物理学 · 物理学 2009-10-31 Jason Melbourne , Ata Sarajedini , Andrew Layden , Donald H. Martins

Thanks to the outstanding capabilites of the HST, our current knowledge about the M31 globular clusters (GCs) is similar to our knowledge of the Milky Way GCs in the 1960s-1970s, which set the basis for studying the halo and galaxy…

High precision trigonometric parallaxes from the HIPPARCOS satellite and accurate metal abundances ([Fe/H], [O/Fe], and [alpha/Fe]) from high resolution spectroscopy for about 30 local subdwarfs have been used to derive distances and ages…

天体物理学 · 物理学 2007-05-23 R. G. Gratton , F. Fusi Pecci , E. Carretta , G. Clementini , C. E. Corsi , M. G. Lattanzi

We present mean horizontal branch absolute magnitudes and iron abundances for a sample of 39 globular clusters. These quantities were calculated in an unprecedented homogeneous fashion based on Fourier decomposition of ligt curves of RR…

太阳与恒星天体物理 · 物理学 2023-06-05 Armando Arellano Ferro

We have derived accurate distances to Galactic globular clusters by combining data from the Gaia Early Data Release 3 with distances based on Hubble Space telescope HST data and literature based distances. We determine distances either…

星系天体物理 · 物理学 2021-07-14 Holger Baumgardt , Eugene Vasiliev

A catalog including a set of the most recent Color Magnitude Diagrams (CMDs) is presented for a sample of 61 Galactic Globular Clusters (GGCs). We used this data-base to perform an homogeneous systematic analysis of the evolved sequences…

天体物理学 · 物理学 2010-02-18 F. R. Ferraro , M. Messineo , F. Fusi Pecci , M. A. De Palo , O. Straniero , A. Chieffi , M. Limongi

We present the complete photometric database and the color-magnitude diagrams for 74 Galactic globular clusters observed with the HST/WFPC2 camera in the F439W and F555W bands. A detailed discussion of the various reduction steps is also…

We present deep VI photometry of stars in the globular cluster M5 (NGC 5904) based on images taken with the Hubble Space Telescope. The resulting color-magnitude diagram reaches below V ~ 27 mag, revealing the upper 2-3 magnitudes of the…

天体物理学 · 物理学 2009-11-13 Andrew C. Layden , Ata Sarajedini , Ted von Hippel , Adrienne M. Cool

We present new UV (F218W) data for stars in the central region of the Galactic globular cluster NGC2808, collected with the WFPC2 camera on board of the Hubble Space Telescope. These data together with F439W and F555W-band data and previous…

天体物理学 · 物理学 2009-11-11 V. Castellani , G. Iannicola , G. Bono , M. Zoccali , S. Cassisi , R. Buonanno

We review the results on distances and absolute ages of galactic globular clusters (GCs) obtained after the release of the Hipparcos catalogue. Several methods for the Population II local distance scale are discussed, exploiting NEW RESULTS…

天体物理学 · 物理学 2009-10-31 Eugenio Carretta , Raffaele Gratton , Gisella Clementini , Flavio Fusi Pecci

In this paper we present the second and final part of a large and photometrically homogeneous CCD color-magnitude diagram (CMD) data base, comprising 52 nearby Galactic globular clusters (GGC) imaged in the V and I bands. The catalog has…

天体物理学 · 物理学 2015-06-24 A. Rosenberg , A. Aparicio , I. Saviane , G. Piotto

Single epoch K-band photometry of 32 RR Lyrae stars in the young galactic globular cluster IC4499 is presented. The mean magnitudes have been estimated using the K-band template light-curves of Jones, Carney and Fulbright (1996). We derive…

天体物理学 · 物理学 2009-11-10 Jesper Storm
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