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20052018
most citedCircumstellar Disk Lifetimes In Numerous Galactic Young Stellar Clusters

129 citations · 244 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2018★ 129 cited

Circumstellar Disk Lifetimes In Numerous Galactic Young Stellar Clusters

Alexander J. W. Richert, Konstantin V. Getman, Eric D. Feigelson +5

Photometric detections of dust circumstellar disks around pre-main sequence (PMS) stars, coupled with estimates of stellar ages, provide constraints on the time available for plane…

astro-ph.GA2018★ 29 cited

Young Star Clusters In Nearby Molecular Clouds

Konstantin V. Getman, Michael A. Kuhn, Eric D. Feigelson +3

The SFiNCs (Star Formation in Nearby Clouds) project is an X-ray/infrared study of the young stellar populations in 22 star forming regions with distances <=1 kpc designed to exten…

astro-ph.SR2015★ 17 cited

PHL 1445: An eclipsing cataclysmic variable with a substellar donor near the period minimum

M. J. McAllister, S. P. Littlefair, I. Baraffe +14

We present high-speed, three-colour photometry of the eclipsing dwarf nova PHL 1445, which, with an orbital period of 76.3 min, lies just below the period minimum of ~82 min for ca…

astro-ph2007

The ultra-compact binary candidate KUV 23182+1007 is a bright quasar

John Southworth, A. Schwope, B. T. Gaensicke +1

KUV 23182+1007 was identified as a blue object in the Kiso UV Survey in the 1980s. Classification-dispersion spectroscopy showed a featureless continuum except for a strong emissio…

astro-ph2006★ 24 cited

SDSSJ212531.92-010745.9 - the first definite PG1159 close binary system

T. Nagel, S. Schuh, D. -J. Kusterer +5

The archival spectrum of SDSSJ212531.92-010745.9 shows not only the typical signature of a PG1159 star, but also indicates the presence of a companion. Our aim was the proof of the…

astro-ph2005★ 45 cited

Outflowing disk formation in B[e] supergiants due to rotation and bi--stability in radiation driven winds

M. Cure, D. F. Rial, L. Cidale

The effects of rapid rotation and bi-stability upon the density contrast between the equatorial and polar directions of a B[e] supergiant are re-investigated. Based upon a new slow…