activity
19982019
most citedA Catalog of Diffuse Interstellar Bands in the Spectrum of HD 204827

258 citations · 1k across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2019★ 98 cited

The Apache Point Observatory Catalog of Optical Diffuse Interstellar Bands

Haoyu Fan, L. M. Hobbs, Julie A. Dahlstrom +7

Aiming for a new and more comprehensive DIB catalog between 4,000 and 9,000Å, we revisited the Atlas Catalog based on the observations of HD 183143 and HD 204827 (Hobbs et al. 2008…

astro-ph.GA2017★ 33 cited

The Behavior of Selected Diffuse Interstellar Bands with Molecular Fraction in Diffuse Atomic and Molecular Clouds

Haoyu Fan, Daniel E. Welty, Donald G. York +10

We study the behavior of eight diffuse interstellar bands (DIBs) in different interstellar environments, as characterized by the fraction of hydrogen in molecular form [(H)]…

astro-ph.SR2012★ 38 cited

Geometry and velocity structure of HD 44179's bipolar jet

Joshua D. Thomas, Adolf N. Witt, Jason P. Aufdenberg +4

In this paper we analyse a set of 33 optical spectra, which were acquired with the ARCES echelle spectrograph (R = 38,000) on the 3.5-m telescope at the Apache Point Observatory. W…

astro-ph.SR2011★ 9 cited

The nature of the Na I D-lines in the Red Rectangle

Joshua D. Thomas, Adolf N. Witt, Jason P. Aufdenberg +6

In this paper we examine the profiles of the complex Na I D-lines in the Red Rectangle. The spectra were acquired with the ARCES échelle spectrograph R = 38,000 on the 3.5-m telesc…

astro-ph.SR2010★ 30 cited

Li I and K I Scatter in Cool Pleiades Dwarfs

J. R. King, S. C. Schuler, L. M. Hobbs +1

We utilize high-resolution (R~60,000), high S/N (~100) spectroscopy of 17 cool Pleiades dwarfs to examine the confounding star-to-star scatter in the 6707 Li I line strengths in th…

astro-ph.GA2009★ 220 cited

Studies of the Diffuse Interstellar Bands. III. HD 183143

L. M. Hobbs, D. G. York, J. A. Thorburn +8

Echelle spectra of HD 183143 [B7Iae, E(B-V) = 1.27] were obtained on three nights, at a resolving power R = 38,000 and with a signal-to-noise ratio ~1000 at 6400 A in the final, co…