Search Results - (Author, Cooperation:H. Spinrad)
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1F. Walter ; R. Decarli ; C. Carilli ; F. Bertoldi ; P. Cox ; E. Da Cunha ; E. Daddi ; M. Dickinson ; D. Downes ; D. Elbaz ; R. Ellis ; J. Hodge ; R. Neri ; D. A. Riechers ; A. Weiss ; E. Bell ; H. Dannerbauer ; M. Krips ; M. Krumholz ; L. Lentati ; R. Maiolino ; K. Menten ; H. W. Rix ; B. Robertson ; H. Spinrad ; D. P. Stark ; D. Stern
Nature Publishing Group (NPG)
Published 2012Staff ViewPublication Date: 2012-06-16Publisher: Nature Publishing Group (NPG)Print ISSN: 0028-0836Electronic ISSN: 1476-4687Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsPublished by: -
2Staff View
ISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] We have obtained a good quality spectrum of the candidate object3 (Fig. 1) on the night of 9 May 1983 UT, using CRYOCAM charge coupled device (CCD) spectrograph on the Kitt Peak 4-m telescope. Very heavy extinction is evident. We have clearly detected Ha in absorption, but the sodium D lines are ...Type of Medium: Electronic ResourceURL: -
3Kulkarni, S. R. ; Djorgovski, S. G. ; Eichelberger, A. C. ; Côté, P. ; Blakeslee, J. P. ; Odewahn, S. C. ; Harrison, F. A. ; Frail, D. A. ; Filippenko, A. V. ; Leonard, D. C. ; Riess, A. G. ; Spinrad, H. ; Stern, D. ; Bunker, A. ; Dey, A. ; Grossan, B. ; Perlmutter, S. ; Knop, R. A. ; Hook, I. M. ; Feroci, M. ; Bloom, J. S.
[s.l.] : Macmillian Magazines Ltd.
Published 1999Staff ViewISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] Cosmic γ-ray bursts have now been firmly established as one of the most powerful phenomena in the Universe, releasing almost the rest-mass energy of a neutron star within the space of a few seconds (ref. 1). The two most popular models to explain γ-ray bursts are ...Type of Medium: Electronic ResourceURL: -
4Staff View
ISSN: 0019-1035Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: PhysicsType of Medium: Electronic ResourceURL: -
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ISSN: 0019-1035Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: PhysicsType of Medium: Electronic ResourceURL: -
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ISSN: 0019-1035Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: PhysicsType of Medium: Electronic ResourceURL: -
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ISSN: 0019-1035Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: PhysicsType of Medium: Electronic ResourceURL: -
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ISSN: 0019-1035Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: PhysicsType of Medium: Electronic ResourceURL: -
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ISSN: 0019-1035Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: PhysicsType of Medium: Electronic ResourceURL: -
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ISSN: 0019-1035Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: PhysicsType of Medium: Electronic ResourceURL: -
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ISSN: 0019-1035Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: PhysicsType of Medium: Electronic ResourceURL: -
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ISSN: 0019-1035Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: PhysicsType of Medium: Electronic ResourceURL: -
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ISSN: 0019-1035Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: PhysicsType of Medium: Electronic ResourceURL: -
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ISSN: 0019-1035Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: PhysicsType of Medium: Electronic ResourceURL: -
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ISSN: 1573-0794Source: Springer Online Journal Archives 1860-2000Topics: GeosciencesPhysicsNotes: Abstract The spectral synthesis of C 2 Swan band sequence δV = − 1 indicates the intensity of the forbidden green oxygen line of 5577.3 ⫗ to be about 3 to 5% of the 6300 ⫗ line. Therefore, it appears that the green line should be observable in high-resolution spectra of a bright comet. Festou and Feldman suggest red/green 〉/ 10 means a water parent origin.Type of Medium: Electronic ResourceURL: -
16McCARTHY, D. ; STOLOVY, S. ; KERN, S. ; SCHNEIDER, G. ; FERRO, A. ; SPINRAD, H. ; BLACK, J. ; SMITH, B.
Springer
Published 1997Staff ViewISSN: 1573-0794Source: Springer Online Journal Archives 1860-2000Topics: GeosciencesPhysicsNotes: Abstract Near-infrared images of comet Hale-Bopp (C/1995 O1) were obtained from NICMOS/HST on UT August 27–28, 1997, when the comet emerged from the 50 degree solar elongation limit at 2.99 AU from Earth. Diffraction-limited images were obtained with camera 2 filters centered at 1.87, 1.90, 2.04 and 2.22 μm with ∼0.2″ resolution (0.076″/pixel; 165 km/pixel). Over the 1.7-hour baseline of observation, a recent (〈7 hours) outburst is seen in the form of an expanding spiral arm with a projected expansion velocity of ∼80 m/s. Other asymmetric features include a jet emanating from the nucleus and several static linear features. Comparisons of the flux distribution in the 2.04 and 2.22 μm filters indicate that the region near the nucleus exhibits a slight, ∼3%, water ice absorption.Type of Medium: Electronic ResourceURL: