Variability of High Luminosity Stars - CYC2HIGH

Details Variability of High Luminosity Stars - CYC2HIGH Variability of High Luminosity Stars - CYC2HIGH

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993hst..prop.4946b&link_type=abstract

HST Proposal ID #4946

Physics

Hst Proposal Id #4946

Scientific paper

Some of the most luminous and massive stars in our galaxy and in the Large Magellanic Cloud will be monitored for variability in light. Knowledge of the time scales and amplitudes of luminosity fluctuations can perhaps place useful constraints on various stellar models. Revision History: Received on RPS 9/1/89; Added to SCCS 9/5/89 RPSS V7.2 remote & local - SALM 9/8/89; Text changes & added ACQ to repeat visits - SALM 9/28/89; Move 9 targ to cycle2 - SALM 2/14/90 Move 3 targ to cycle 2; add UV2 obs for P-CYG - SALM 3/26/90; Expanded illegally nested repeat - SALM 6/21/90; Moved REPEAT to USE - SALM 6/28/90; Defer all targets to cycle 1--BJW 11/26/90; Split proposal by cycle--BJW 3/22/91; Changes to observations of HD193237--BJW 6/19/91; Update target list--BJW 6/27/91; Resubmitted proposal with PRISM mode observations-- BJW 6/25/92;

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