G
G. Neugebauer
Researcher at University of Arizona
Publications - 387
Citations - 24341
G. Neugebauer is an academic researcher from University of Arizona. The author has contributed to research in topics: Galaxy & Quasar. The author has an hindex of 73, co-authored 387 publications receiving 23703 citations. Previous affiliations of G. Neugebauer include Jet Propulsion Laboratory & University of Hawaii.
Papers
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Journal ArticleDOI
A new luminosity component in 3C 48
TL;DR: In this article, it was shown that the infrared emission from the 3C48 quasar is most likely not an extension of the radio emission of the quasar, but thermal radiation arising in a highly luminous galaxy surrounding it.
Journal ArticleDOI
Multifrequency observations of BL Lacertae in 1988
Nobuyuki Kawai,M. Matsuoka,Joel N. Bregman,Hugh D. Aller,Margo F. Aller,Philip A. Hughes,Steven A. Balbus,Thomas J. Balonek,K. C. Chambers,R. E. S. Clegg,S. D. Clements,R. J. Leacock,Alex G. Smith,Joseph S. Miller,Mark Hereld,Melvin Hoare,V. A. Hughes,George K. Miley,G. H. Moriarty-Schieven,Keith Matthews,G. Neugebauer,Takaya Ohashi,Patrick F. Roche,Harley A. Thronson,E. Valtaoja,H. Teräsranta,James R. Webb,R. Goodrich,Beverley J. Wills,Derek Wills +29 more
TL;DR: In this paper, simultaneous multi-wavelength observations of BL Lacertae were performed on two occasions separated by month in 1988 June and July, covering the radio, submillimeter, infrared, optical, ultraviolet, and X-ray wave bands.
Journal ArticleDOI
Far-infrared observations of IRC + 10216
M. P. Campbell,Paul M. Harvey,William F. Hoffmann,J. H. Elias,G. Neugebauer,D. Y. Gezari,W. E. Westbrook,H. S. Hudson,B. T. Soifer,Michael W. Werner +9 more
TL;DR: In this paper, photometric observations of IRC + 10216 in five wavelength intervals from 50 to 1000 μ are reported, where the observed radiation is interpreted as thermal emission from dust in the extended molecular cloud heated by the compact 2-20 μ source as the core of the cloud.
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Further joint X-ray, infrared, and radio observations of Cygnus X-3
K. O. Mason,P. W. Sanford,E. E. Becklin,J. H. Elias,G. Neugebauer,L. Blankenship,Robert L. Brown,Robert M. Hjellming,Keith Matthews,Paul Murdin +9 more
TL;DR: The radio fluxes were usually low during the period of observation; both the daily average radio flux levels and spectral index remained nearly constant as discussed by the authors, and the X-ray data showed the periodic structure which is typical of Cygnus X-3.