activity
20072020
most citedThe CO Molecular Outflows of IRAS 16293-2422 Probed by the Submillimeter Array

53 citations · 113 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.EP202025 cited

A Characterization of the Circumstellar Gas around WD 1124-293 using Cloudy

Amy Steele, John Debes, Siyi Xu +2

Between 30 - 50% of white dwarfs (WDs) show heavy elements in their atmospheres. This "pollution" is thought to arise from the accretion of planetesimals perturbed by outer planet(…

astro-ph.SR201920 cited

Background Infrared Sources for Studying the Galactic Center's Interstellar Gas

T. R. Geballe, E. Lambrides, B. Schlegelmilch +5

We briefy describe the results of a K-band spectroscopic survey of over 500 highly reddened point-like objects on sightlines toward the Central Molecular Zone (CMZ) of the Galaxy.…

astro-ph.GA2018

Super-Eddington Accretion in the WISE-Selected Extremely Luminous Infrared Galaxy W2246-0526

Chao-Wei Tsai, Peter Eisenhardt, Hyunsung Jun +8

We use optical and near-infrared spectroscopy to observe rest-UV emission lines and estimate the black hole mass of WISEA J224607.56-052634.9 (W2246-0526) at z = 4.601, the most lu…

astro-ph.GA2018

The MALATANG Survey: the L_gas-L_IR correlation on sub-kiloparsec scale in six nearby star-forming galaxies as traced by HCN J=4-3 and HCO^+ J=4-3

Qing-Hua Tan, Yu Gao, Zhi-Yu Zhang +43

We present HCN J=4-3 and HCO^+ J=4-3 maps of six nearby star-forming galaxies, NGC 253, NGC 1068, IC 342, M82, M83, and NGC 6946, obtained with the James Clerk Maxwell Telescope as…

astro-ph.GA201515 cited

Molecular and Ionized Hydrogen in 30 Doradus. I. Imaging Observations

Sherry C. C. Yeh, Ernest R. Seaquist, Christopher D. Matzner +1

We present the first fully calibrated H, 1-0 S(1) image of the entire 30 Doradus nebula. The observations were conducted using the NOAO Extremely Wide-Field Infrared Imager on…

astro-ph200753 cited

The CO Molecular Outflows of IRAS 16293-2422 Probed by the Submillimeter Array

Sherry C. C. Yeh, Naomi Hirano, Tyler L. Bourke +4

We have mapped the proto-binary source IRAS 16293-2422 in CO 2-1, 13CO 2-1, and CO 3-2 with the Submillimeter Array (SMA). The maps with resolution of 1".5-5" reveal a single small…