SUMMARY OF PROPOSAL 82022

DR MICHAEL F. CORCORAN
CORCORAN@BARNEGAT.GSFC.NASA.GOV

GSFC/USRA
CODE 662 GSFC
GREENBELT
MD USA 20771
Tel: 301-286-5576 Fax: 301-286-1629
Medium: CD ROM
Subject: STARS

LONG TERM MONITORING OF THE SHORT PERIOD COLLIDING WIND BINARY SYSTEM V444 CYGNI


ABSTRACT

We propose to monitor the important short period (4.2 day) binary system V444~Cyg for two weeks with ASCA, to provide coverage over 3 complete orbital cycles. These observations will provide the most detailed orbital lightcurve of any colliding wind system, and determine the extent of any non phase related variability. V444~Cyg is of particular importance in that it is the best example of a short period colliding wind binary system, and is a key testing ground for our understanding of wind-wind interactions, W-R winds and W-R stars in general.

CO-INVESTIGATORS
CO-I NAME INSTITUTE COUNTRY
IAN STEVENSBIRMINGHAMUK
ANDY POLLOCKC&S LTDUK
THE XMEGA GROUPVARIOUSUSA

TARGETS

TARGET NAMEPRIRADECTIMETCOFFGISSIS CNTOBS
1)V444 CYG
B
304.8850 38.7317
500 ks
N
N
P
0.02000
1