Search Results - (Author, Cooperation:P. M. Harvey)
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1Latest Papers from Table of Contents or Articles in PressB. L. de Vries ; B. Acke ; J. A. Blommaert ; C. Waelkens ; L. B. Waters ; B. Vandenbussche ; M. Min ; G. Olofsson ; C. Dominik ; L. Decin ; M. J. Barlow ; A. Brandeker ; J. Di Francesco ; A. M. Glauser ; J. Greaves ; P. M. Harvey ; W. S. Holland ; R. J. Ivison ; R. Liseau ; E. E. Pantin ; G. L. Pilbratt ; P. Royer ; B. Sibthorpe
Nature Publishing Group (NPG)
Published 2012Staff ViewPublication Date: 2012-10-06Publisher: Nature Publishing Group (NPG)Print ISSN: 0028-0836Electronic ISSN: 1476-4687Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsPublished by: -
2Articles: DFG German National LicensesBeichman, C. A. ; Neugebauer, G. ; Soifer, B. T. ; Wootten, H. A. ; Roellig, T. ; Harvey, P. M.
[s.l.] : Nature Publishing Group
Published 1981Staff ViewISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] The radio source 1413 + 135 is shown to be one of the strongest known emitters of millimetre radiation. The energy distribution of this object measured between metre and X-ray wavelengths reveals that most of the power emitted by this object comes out at millimetre and far-IR wavelengths. If ...Type of Medium: Electronic ResourceURL: -
3Articles: DFG German National LicensesStaff View
ISSN: 1572-946XSource: Springer Online Journal Archives 1860-2000Topics: PhysicsNotes: Abstract We present 50 and 100µm photometry and size information for several main sequence stars surrounded by dust shells. The observations from NASA's Kuiper Airborne Observatory include the “Vega-like” stars, Beta Pic, Fomalhaut, as well as four stars suggested by Walker and Wolstencroft to belong possibly to the same class. The results of our observations are best interpreted as upper limits to the far-infrared sizes of the dust clouds around all of the stars except Fomalhaut and Beta Pic. We have also fit simple, optically thin models to the Beta Pic data to explore the range of shell parameters consistent with our limits and with previous observations.Type of Medium: Electronic ResourceURL: