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20022023
most citedLooking for Pure Rotational H_2 Emission from Protoplanetary Disks

58 citations · 505 across the 24 of their papers we have counts for

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12 papers · 1 filter

astro-ph2008★ 55 cited

The TEXES Survey For H2 Emission From Protoplanetary Disks

M. A. Bitner, M. J. Richter, J. H. Lacy +9

We report the results of a search for pure rotational molecular hydrogen emission from the circumstellar environments of young stellar objects with disks using the Texas Echelon Cr…

astro-ph2008★ 24 cited

Mg I emission lines at 12 and 18 micrometer in K giants

J. O. Sundqvist, N. Ryde, G. M. Harper +2

The solar Mg I emission lines at 12 micrometer have already been observed and analyzed well. Previous modeling attempts for other stars have, however, been made only for Procyon an…

astro-ph2008★ 2 cited

A potential new method for determining the temperature of cool stars

S. Viti, H. R. A. Jones, M. J. Richter +3

We present high resolution (R = 90,000) mid-infrared spectra of M dwarfs. The mid infrared region of the spectra of cool low mass stars contain pure rotational water vapour transit…

astro-ph2007★ 34 cited

TEXES Observations of Pure Rotational H2 Emission From AB Aurigae

M. A. Bitner, M. J. Richter, J. H. Lacy +3

We present observations of pure rotational molecular hydrogen emission from the Herbig Ae star, AB Aurigae. Our observations were made using the Texas Echelon Cross Echelle Spectro…

astro-ph2007★ 20 cited

W51 IRS 2: A Massive Jet Emerging from a Molecular Cloud into an H II Region

J. H. Lacy, D. T. Jaffe, Q. Zhu +6

We have mapped [Ne II] (12.8um) and [S IV] (10.5um) emission from W51 IRS 2 with TEXES on Gemini North, and we compare these data to VLA free-free observations and VLT near-infrare…

astro-ph2006★ 11 cited

High Resolution Mid-Infrared Imaging of Radio Ultra-Compact HII Regions

Uriel Giveon, Matthew J. Richter, Robert H. Becker +1

We present data from mid-infrared Keck Telescope imaging of 18 radio-selected ultra-compact HII region candidates at diffraction-limited resolution. The goal of these observations…