output
20042009
most citedCats and Dogs, Hair and A Hero: A Quintet of New Milky Way Companions

810 citations

Showing 2006Show all

34 papers · 1 filter

astro-ph200630 cited

HST and Optical Observations of Three Pulsating Accreting White Dwarfs in Cataclysmic Variables

Paula Szkody, Anjum Mukadam, Boris T. Gaensicke +8

Ultraviolet observations using the Solar Blind Channel on the Hubble Space Telescope provide light curves and low resolution spectra of three pulsating white dwarfs in the cataclys…

astro-ph200634 cited

Investigating the Nature of Variable Class I and Flat Spectrum Protostars Using 2-4m Spectroscopy

Tracy L. Beck

In this study I present new K and L-band infrared photometry and 2-4m spectra of ten Class I and flat spectrum stars forming within the Taurus dark cloud complex. Nine source…

astro-ph200636 cited

Gemini Spectroscopic Survey of Young Star Clusters in Merging/Interacting Galaxies. I. NGC 3256 Tidal-Tail Clusters

Gelys Trancho, Nate Bastian, Francois Schweizer +1

We present Gemini optical spectroscopy of three young star clusters in the western tidal tail of NGC3256. Compact star clusters (as opposed to dwarf-galaxy candidates) in tidal tai…

astro-ph200623 cited

The Structure of the Inner HH 34 Jet from Optical Integral Field Spectroscopy

Tracy L. Beck, A. Riera, A. C. Raga +1

We present high spatial resolution optical integral field spectroscopy of a collimated Herbig-Haro jet viewed nearly edge-on. Maps of the line emission, velocity centroid, and velo…

astro-ph200692 cited

Trigonometric Parallaxes of Central Stars of Planetary Nebulae

Hugh C. Harris, Conard C. Dahn, Blaise Canzian +11

Trigonometric parallaxes of 16 nearby planetary nebulae are presented, including reduced errors for seven objects with previous initial results and results for six new objects. The…

astro-ph200619 cited

Spectropolarimetry of the 3.4 micron absorption feature in NGC 1068

R. E. Mason, G. S. Wright, A. Adamson +1

In order to test the silicate-core/organic-mantle model of galactic interstellar dust, we have performed spectropolarimetry of the 3.4 micron C-H bond stretch that is characteristi…