activity
19992016
most citedThe ACS Survey of Galactic Globular Clusters. XII. Photometric Binaries along the Main-Sequence

484 citations · 1.4k across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2016★ 19 cited

The Proper Motion of Pyxis: the first use of Adaptive Optics in tandem with HST on a faint halo object

Tobias K. Fritz, Sean T. Linden, Paul Zivick +13

We present a proper motion measurement for the halo globular cluster Pyxis, using HST/ACS data as the first epoch, and GeMS/GSAOI Adaptive Optics data as the second, separated by a…

astro-ph.SR2011★ 484 cited

The ACS Survey of Galactic Globular Clusters. XII. Photometric Binaries along the Main-Sequence

A. P. Milone, G. Piotto, L. R. Bedin +15

The fraction of binary stars is an important ingredient to interpret globular cluster dynamical evolution and their stellar population. We investigate the properties of main-sequen…

astro-ph2008★ 104 cited

Tombaugh 2: The First Open Cluster with a Significant Abundance Spread or Embedded in a Cold Stellar Stream?

P. M. Frinchaboy, A. F. Marino, S. Villanova +3

We present new abundances and radial velocities for stars in the field of the open cluster Tombaugh 2, which has been suggested to be associated with the Galactic Anticenter Stella…

astro-ph2007★ 298 cited

The ACS Survey of Galactic Globular Clusters. III. The Double Subgiant Branch of NGC 1851

A. P. Milone, L. R. Bedin, G. Piotto +13

Photometry with HST's ACS reveals that the subgiant branch (SGB) of the globular cluster NGC 1851 splits into two well-defined branches. If the split is due only to an age effect,…

astro-ph2002★ 235 cited

Starcounts Redivivus. IV. Density Laws Through Photometric Parallaxes

M. H. Siegel, S. R. Majewski, I. N. Reid +1

In an effort to more precisely define the spatial distribution of Galactic field stars, we present an analysis of the photometric parallaxes of 70,000 stars covering nearly 15 squa…

astro-ph1999★ 8 cited

Omega Centauri: Nucleus of a Milky Way Dwarf Spheroidal?

S. R. Majewski, R. J. Patterson, D. I. Dinescu +4

We focus on two aspects of Omega Cen that are rather uncharacteristic of globular clusters: its metallicity distribution and its orbit. We use (1) a Washington (M-T_2,M)_o color-ma…