Cornelia C. Lang, Ph.D.
Affiliations: | 2000 | University of California, Los Angeles, Los Angeles, CA |
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"Cornelia Lang"Mean distance: 17.6 | S | N | B | C | P |
Parents
Sign in to add mentor| Mark Morris | grad student | 2000 | UCLA | |
| (A radio study of the Galactic center Arched Filament complex.) | ||||
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Publications
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| Butterfield NO, Ginsburg A, Ludovici DA, et al. (2020) 6.7 GHz CH3OH Absorption toward the N3 Galactic Center Point Source The Astrophysical Journal. 889: 174 |
| Paré DM, Lang CC, Morris MR, et al. (2019) A VLA Polarimetric Study of the Galactic Center Radio Arc: Characterizing Polarization, Rotation Measure, and Magnetic Field Properties The Astrophysical Journal. 884: 170 |
| Butterfield N, Lang CC, Morris M, et al. (2017) M0.20–0.033: An Expanding Molecular Shell in the Galactic Center Radio Arc The Astrophysical Journal. 852: 11 |
| Fu H, Hennawi JF, Prochaska JX, et al. (2016) THE CIRCUMGALACTIC MEDIUM OF SUBMILLIMETER GALAXIES. I. FIRST RESULTS FROM A RADIO-IDENTIFIED SAMPLE The Astrophysical Journal. 832: 52 |
| Ludovici DA, Lang CC, Morris MR, et al. (2016) THE UNUSUAL GALACTIC CENTER RADIO SOURCE N3 Astrophysical Journal. 826 |
| Mills EAC, Butterfield N, Ludovici DA, et al. (2015) ABUNDANT CH |
| Cseh D, Kaaret P, Corbel S, et al. (2014) Unveiling recurrent jets of the ULX holmberg II X-1: Evidence for a massive stellar-mass black hole? Monthly Notices of the Royal Astronomical Society: Letters. 439: L1-L5 |
| Marlowe H, Kaaret P, Lang C, et al. (2014) Spectral state transitions of the Ultraluminous X-ray Source IC 342 X-1 Monthly Notices of the Royal Astronomical Society. 444: 642-650 |
| Cseh D, Corbel S, Kaaret P, et al. (2012) Black Hole Powered Nebulae And A Case Study Of The Ultraluminous X-Ray Source Ic 342 X-1 The Astrophysical Journal. 749: 17 |
| Richards EE, Lang CC, Trombley C, et al. (2012) Multiwavelength observations of massive stellar cluster candidates in the galaxy Astronomical Journal. 144 |