Zobrazeno 1 - 10
of 56
pro vyhledávání: '"R. F. Knacke"'
Autor:
S. B. Peschke, Humberto Campins, T. Y. Brooke, Manfred Stickel, Eberhard Grün, H. U. Keller, J. Crovisier, M. Solc, V. Vanysek, John C. Zarnecki, David J. Osip, Mark V. Sykes, R. F. Knacke, Dietrich Lemke, Carey M. Lisse, Michael Müller, I. Heinrichsen, Philippe Lamy, Ch. Leinert, Harald Krüger, H. Boehnhardt, Martha S. Hanner, T. G. Muller, C. Delahodde
Publikováno v:
Scopus-Elsevier
Comet Hale-Bopp was observed five times with ISOPHOT, the photometer on board ESA's Infrared Space Observatory (ISO) between 4.6 and 2.8 AU. Each time, broadband photometry was performed using 4 different detectors, 5 apertures and 10 filters coverin
Autor:
H. A. Thronson, J. K. Davies, J. Hackwell, T. G. Hawarden, R. F. Knacke, D. Lester, C. M. Mountain
Publikováno v:
Space Science Reviews. 61:145-169
Autor:
R. F. Knacke
Publikováno v:
Molecular Clouds in the Milky Way and External Galaxies ISBN: 9783540504382
Present evidence for where and in what forms the abundant elements O, C, N, Si, Mg, Fe, and S occur in molecular clouds is reviewed. Studies of both gas and dust show that most of the elements, with the probable exception of N, are far below cosmic a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::55f4a11a4f30545e846c0ecdbe8f6392
https://doi.org/10.1007/3-540-50438-9_253
https://doi.org/10.1007/3-540-50438-9_253
Publikováno v:
Molecular Clouds in the Milky Way and External Galaxies ISBN: 9783540504382
Searches for the R(O) line of the CH4v3 band at 3.3 μm give CH4/CO ≤3.3 x 10−2 in AFGL 961 (Rosette Nebula) and ≤2.4 x 10−3 in AFGL 989 (NGC 2264). The results are consistent with ion-molecule models, but the observations may not sample regi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ab0126367ab8faed1c7af3e5f1c4374a
https://doi.org/10.1007/3-540-50438-9_261
https://doi.org/10.1007/3-540-50438-9_261
Publikováno v:
Icarus. 124(2)
We have measured the spectrum of Titan near 5 micrometers and have found it to be dominated by absorption from the carbon monoxide 1-0 vibration-rotation band. The position of the band edge allows us to constrain the abundance of CO in the atmosphere
Autor:
C. M. Mountain, D. Lester, John K. Davies, T. G. Hawarden, J. Hackwell, R. F. Knacke, Harley A. Thronson
Publikováno v:
Next Generation Infrared Space Observatory ISBN: 9789401051866
EDISON, a large-aperture, radiatively-cooled telescope, is proposed as the major international mission to follow the current generation of cryogenically-cooled infrared space telescopes. It is being studied at present as a 2.5–3.5 m mixed radiative
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::42a1da800f65ac6c1edf5b3af66f2b69
https://doi.org/10.1007/978-94-011-2680-9_13
https://doi.org/10.1007/978-94-011-2680-9_13
Autor:
R. F. Knacke, Charles M. Telesco
Publikováno v:
The Astrophysical Journal. 372:L29
A broad 10-micron emission feature has been detected within 3 arcsec of the star Beta Pic which is known to have a circumstellar, possibly protoplanetary, disk. The observations were made using four narrow-band filters in the MSFC bolometer array at
Publikováno v:
The Astronomical Journal. 101:268
The 3.4 micron emission feature due to cometary organics was detected in Comets P/Brorsen-Metcalf and Okazaki-Levy-Rudenko (1989r). Features-to-continuum ratios in these two comets were higher than those expected from the trend seen in other comets t
Publikováno v:
Astrophysics and Space Science. 35:97-115
Autor:
A. Zaikowski, R. F. Knacke
Publikováno v:
Astrophysics and Space Science. 37:3-9
Infrared spectra (7–40 μ) of the carbonaceous chondrites, Cold Bokkeveld, Murray, and Orgueil are compared with phyllosilicate minerals and interstellar grain spectra. Similarities in the position and shape of the silicate feature near 9.8 μ sugg