subject: Re*2: PG2300+166
Dear Dr. Fred Ringwald,
I have just seen your abstract in PASP. I would be grateful if you
can send me a copy of your forthcoming papers. My postal address is:
Taichi Kato
Dept. of Astronomy, Faculty of Science,
Kyoto University
Oiwake-cho, Kitashirakawa, Sakyo-ku, Kyoto-shi,
Kyoto 606-01
JAPAN
Concerning PG2300+166, did you record the magnitude when you took a
spectrum (or may be guessed from the required exposure time)? If the
object is really a precataclysmic binary, and the object was in a bright
phase (not in an eclipse), it may display narrow emission lines arising
from the secondary facing the hot subdwarf. If your spectrum showed
a subdwarf without peculiarities, it seems to be a single subdwarf.
I would like to know your opinion.
Regards,
Taichi Kato

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