George A. Moellenbrock
Affiliations: | 1997 | Physics | Brandeis University, Waltham, MA, United States |
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Publications
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Bianchi E, Chandler CJ, Ceccarelli C, et al. (2020) FAUST I. The hot corino at the heart of the prototypical Class I protostar L1551 IRS5 Monthly Notices of the Royal Astronomical Society: Letters. 498: L87-L92 |
Hull CLH, Cortes PC, Gouellec VJML, et al. (2020) Characterizing the accuracy of ALMA linear-polarization mosaics Publications of the Astronomical Society of the Pacific. 132: 94501 |
Lacy M, Baum SA, Chandler CJ, et al. (2020) The Karl G. Jansky Very Large Array Sky Survey (VLASS). Science Case and Survey Design Publications of the Astronomical Society of the Pacific. 132: 035001 |
Nagai H, Nakanishi K, Paladino R, et al. (2016) ALMA Science Verification Data: Millimeter Continuum Polarimetry of the Bright Radio Quasar 3C 286 The Astrophysical Journal. 824: 132 |
Brunthaler A, Reid MJ, Menten KM, et al. (2011) The Bar and Spiral Structure Legacy (BeSSeL) survey: Mapping the Milky Way with VLBI astrometry† Astronomische Nachrichten. 332: 461-466 |
Reid MJ, Menten KM, Zheng XW, et al. (2009) Trigonometric Parallaxes Of Massive Star-Forming Regions. Vi. Galactic Structure, Fundamental Parameters, And Noncircular Motions The Astrophysical Journal. 700: 137-148 |
Moellenbrock GA, Claussen MJ, Goss WM. (2009) A precise distance to iras 00420+5530 via H2O maser parallax with the VLBA Astrophysical Journal. 694: 192-204 |
Dodson R, Fomalont EB, Wiik K, et al. (2008) The VSOP 5 GHz active galactic nucleus survey. V. Imaging results for the remaining 140 sources Astrophysical Journal, Supplement Series. 175: 314-355 |
Scott WK, Fomalont EB, Horiuchi S, et al. (2004) The VSOP 5 GHz active galactic nucleus survey. III. Imaging results for the first 102 sources Astrophysical Journal, Supplement Series. 155: 33-72 |
Horiuchi S, Fomalont EB, Scott WK, et al. (2004) THE VSOP 5 GHz active galactic nucleus survey. IV. The angular size/brightness temperature distribution Astrophysical Journal. 616: 110-122 |