Computer Science
Scientific paper
Jul 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993hst..prop.4274l&link_type=abstract
HST Proposal ID #4274
Computer Science
Hst Proposal Id #4274
Scientific paper
WE PROPOSE TO RECORD GHRS ECHELLE SPECTRA (R=100000) OF VERY IN ORDER TO DETECT AND IDENTIFY LOCAL INTERSTELLAR GAS UV ABS BY MEASURING WITH A PRECISION OF 1KM/S THE DOPPLER-SHIFT OF T AND COMPARING THE RESULTS FOR DIFFERENT DIRECTIONS, THE LOCAL THE SUN IS EMBEDDED, SHOULD BE IDENTIFIED THROUGH RECONSTRUCT VELOCITY VECTOR. AN ESTIMATE OF ITS ELECTRON DENSITY COULD BE MGI/MGII LINE RATIOS. OUR OPTICAL RESULTS HAVE ALREADY SHOWN VERY LIKELY EMBEDDED IN ONE OF TWO IDENTIFIED CLOSE MASSES OF VELOCITIES. VERY RECENT NORTHERN HEMISPHERE OBSERVATIONS OF O TWO FEATURES IN THE PARTICULARLY SIMPLE ANTI-GALACTIC CENTER A VELOCITY VECTOR IN PERFECT AGREEMENT WITH THE RECENT HST-GH TOWARDS CAPELLA BY LINSKY ET AL, PROVIDING FOR THE FIRST TIME BETWEEN UV AND VISIBLE DATA AT THE 1 KM/S SCALE. SINCE LINSKY ONLY ONE COMPONENT IN THE STRONG D, FEII AND MGII UV LINES, T VERY GOOD CANDIDATE FOR THE SOLAR-SYSTEM CLOUD. BUT ONLY A TH DETERMINATION OF THE VELOCITY, AS DONE IN THE VISIBLE, AND AN IDENTIFICATION IN ALL DIRECTIONS, AS WE FAILED TO DO IN THE V THE WEAKNESS OF THE LINES, CAN REALLY PROVE THAT THE SUN IS I GAS.THE FOUND VECTOR CAN THEN BE COMPARED WITH THE SOLAR SYST MOTIONS TO INFER THE DECELERATION OF THE GAS AT THE HELIOSPHE
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