activity
20062009
most citedPreplanetary Nebulae: An HST Imaging Survey and a New Morphological Classification System

182 citations · 431 across the 10 of their papers we have counts for

collaborators

6 papers

astro-ph.GA20092 cited

Understanding Mass-Loss and the late Evolution of Intermediate Mass Stars: Jets, Disks, Binarity, Dust and Magnetic Fields

Raghvendra Sahai, Bruce Balick, Eric Blackman +7

Almost all stars in the 1-8 Msun range evolve through the Asymptotic Giant Branch (AGB), preplanetary nebula (PPN) and planetary nebula (PN) evolutionary phases. Most stars that le…

astro-ph2007182 cited

Preplanetary Nebulae: An HST Imaging Survey and a New Morphological Classification System

Raghvendra Sahai, Mark Morris, Carmen Sánchez Contreras +1

Using the Hubble Space Telescope (HST), we have carried out a survey of candidate preplanetary nebulae (PPNs). We report here our discoveries of objects having well-resolved geomet…

astro-ph200738 cited

The LMC's Top 250: Classification of the Most Luminous Compact 8 micron Sources in the Large Magellanic Cloud

Joel H. Kastner, Stephen L. Thorndike, Paul A. Romanczyk +4

To ascertain the nature of the brightest compact mid-infrared sources in the Large Magellanic Cloud (LMC), we have applied an updated version of the Buchanan et al. (2006) 2MASS-MS…

astro-ph200621 cited

Adaptive Optics Imaging of IRAS 18276-1431: a bipolar pre-planetary nebula with circumstellar "searchlight beams" and "arcs"

C. Sanchez Contreras, D. Le Mignant, R. Sahai +2

We present high-angular resolution images of the post-AGB nebula IRAS18276-1431 (also known as OH17.7-2.0) obtained with the Keck II Adaptive Optics (AO) system in its Natural Guid…

astro-ph200648 cited

A Massive Bipolar Outflow and a Dusty Torus with Large Grains in the Pre-Planetary Nebula IRAS 22036+5306

R. Sahai, K. Young, N. A. Patel +2

We report high angular-resolution (~1") CO J=3--2 interferometric mapping, using the Submillimeter Array (SMA), of IRAS22036+5306 (I22036), a bipolar pre-planetary nebula (PPN) wit…

astro-ph200630 cited

X-ray emission from Planetary Nebulae. I. Spherically symmetric numerical simulations

Matthias Stute, Raghvendra Sahai

(abridged) The interaction of a fast wind with a spherical Asymptotic Giant Branch (AGB) wind is thought to be the basic mechanism for shaping Pre-Planetary Nebulae (PPN) and later…