Variability of High Luminosity Stars - Retake of 1095

Details Variability of High Luminosity Stars - Retake of 1095 Variability of High Luminosity Stars - Retake of 1095

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.3926b&link_type=abstract

HST Proposal ID #3926

Physics

Hst Proposal Id #3926

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; Changed PRISM mode to SINGLE; changed all filters to F152M--BJW 9/3/91;

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