Department of Electrical Engineering, Kyoto University, Kyoto, Japan 20. G. Gardent: Universitt Blaise Pascal , Clermont Ferrand, France 21. A...such as Fortran, reads and writes. Pascal , C, Lisp, and Prolog. In short, it offers continuity. 1. Seclusive PRAM (SPRAM) - concurrent reads Simple SIMD
Institut, Justus - Liebig -Universit’i, D-6300 Giessen, Federal Republic of Germany. Paper presented by K. BLOI. ME5. HIGH RESOLUTION INFRARED...Physikalisch-Chemisches Institut, Justus - Liebig -Universit~t, D-6300 Giessen, West Germany. Chairman After Intermission: Y. S. LI, Department of...Universitat zu Koln, 5000 Kbln, West Germany; R. A. CRESWELL, and M. WINNEWISSER, Physikalisch-Chemisches Institut, Justus Liebig - 9JL Universitat, 6300
Ottawa, Ontario KIA OR6 Canada and B. P. Winnewisser Physikalisch-Chemisches Institut Justus - Liebig -Universitit Giessen Heinrich-Buff-Ring 58 6300...Copenhagen, and Physikalisch-Chemisches Institut, Justus - Liebig - Universit~t Giessen, D-6300 Giessen. Most of the reports in the literature concerning...Ontario, Canada KIA OR6 bphysikalisch-Chemisches Institut, Justus - Liebig Universitat, Giessen, W. Germany An absorption spectrum of the CNO free radical
industrial laboratories to perform the optimization and the development of power PMHFETs. They can also be useful for approach simulations such as quasi two...10-1 IHorinosato-Wakamiya, Atsugi 243-01, Japan ABSTRACT The role of high speed devices in semiconductor industry is changing very rapidly during these...fUr Mikroelektronik, Universitt Linz A-4040 Linz, Austria The trend to higher operating frequencies in commercial and industrial millimeter-wave
McArthur, Barbara E.; Benedict, G. Fritz; Barnes, Rory; Martioli, Eder; Korzennik, Sylvain; Nelan, Ed; Butler, R. Paul
We have used high-cadence radial velocity (RV) measurements from the Hobby-Eberly Telescope with existing velocities from the Lick, Elodie, Harlan J. Smith, and Whipple 60'' telescopes combined with astrometric data from the Hubble Space Telescope Fine Guidance Sensors to refine the orbital parameters and determine the orbital inclinations and position angles of the ascending node of components υ And A c and d. With these inclinations and using M * = 1.31M sun as a primary mass, we determine the actual masses of two of the companions: υ And A c is 13.98+2.3 -5.3 M JUP, and υ And A d is 10.25+0.7 -3.3 M JUP. These measurements represent the first astrometric determination of mutual inclination between objects in an extrasolar planetary system, which we find to be 29fdg9 ± 1°. The combined RV measurements also reveal a long-period trend indicating a fourth planet in the system. We investigate the dynamic stability of this system and analyze regions of stability, which suggest a probable mass of υ And A b. Finally, our parallaxes confirm that υ And B is a stellar companion of υ And A. Based on observations made with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Based on observations obtained with the Hobby-Eberly Telescope, which is a joint project of the University of Texas at Austin, the Pennsylvania State University, Stanford University, Ludwig-Maximilians-Universitt Mnchen, and Georg-August-Universität Göttingen.