output
19932026
most citedThe Seventh Data Release of the Sloan Digital Sky Survey

5.4k citations

Showing 2010 · astro-ph.SRShow all

29 papers · 2 filters

astro-ph.SR2010★ 125 cited

Sodium-Oxygen anticorrelation among Horizontal Branch Stars in the Globular Cluster M4

A. F Marino, S. Villanova, A. P. Milone +4

The horizontal branch (HB) morphology of globular clusters (GC) is mainly governed by metallicity. The second parameter problem, well known since the 60's, states that metallicity…

astro-ph.SR2010★ 39 cited

Are Proto-Planetary Nebulae Shaped by a Binary? Results of a Long-Term Radial Velocity Study

Bruce J. Hrivnak, Wenxian Lu, Katrina Loewe Wefel +4

The shaping of the nebula is currently one of the outstanding unsolved problems in planetary nebula (PN) research. Several mechanisms have been proposed, most of which require a bi…

astro-ph.SR2010★ 112 cited

Supernova 2008bk and Its Red Supergiant Progenitor

Schuyler D. Van Dyk, Tim J. Davidge, Nancy Elias-Rosa +8

We have obtained limited photometric and spectroscopic data for Supernova (SN) 2008bk in NGC 7793, primarily at >~ 150 d after explosion. We find that it is a Type II-Plateau (II-P…

astro-ph.SR2010★ 96 cited

A Submillimeter Array Survey of Protoplanetary Disks in the Orion Nebula Cluster

Rita K. Mann, Jonathan P. Williams

We present the full results of our 3-year long Submillimeter Array survey of protoplanetary disks in the Orion Nebula Cluster. We imaged 23 fields at 880 microns and 2 fields at 13…

astro-ph.SR2010★ 29 cited

Fiducial Stellar Population Sequences for the VJKs Photometric System

Crystal Brasseur, Peter B. Stetson, Don A. VandenBerg +3

We have obtained broad-band near-infrared photometry for seven Galactic star clusters (M92, M15, M13, M5, NGC1851, M71 and NGC6791) using the WIRCam wide-field imager on the Canada…

astro-ph.SR2010★ 34 cited

The Be Star HD 215227: A Candidate Gamma-ray Binary

S. J. Williams, D. R. Gies, R. A. Matson +4

The emission-line Be star HD 215227 lies within the positional error circle of the newly identified gamma-ray source AGL J2241+4454. We present new blue spectra of the star, and we…