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(fwd) PG0943+521 + GROJ0422+32



>From munari@astrpd.DNET.NASA.GOV Sun Jan  9 23:14:45 1994
From: munari@astrpd.DNET.NASA.GOV
To: "tkato@kusastro.kyoto-u.ac.jp"@6913.DNET.NASA.GOV
Subject: RE: CCD observation of GRO J0422+32 etc.
Status: R

Dear dr. Kato,
I would be very interested to receive identification charts for both
GRO J0422+32 and PG 0943+521 as well as photometric comparison sequences.
In coming days and weeks I'll be observing at the 1.8 m telescope in Asiago
with CCD spectrographs. I would be interested to obtain photographic photometry
too with the Schmidt 67/92 cm telescope.
My fax number in Asiago is +39-424-462884.
Best regards
Ulisse Munari

>From far@astro.keele.ac.uk Sun Jan  9 23:59:25 1994
Date: Sun, 9 Jan 1994 14:53:59 +0000 (WET)
From: Fred Ringwald <far@astro.keele.ac.uk>
Subject: Re: CCD observation of GRO J0422+32 etc.
To: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
In-Reply-To: <9401091133.AA21760@sanews.kusastro.kyoto-u.ac.jp>
Message-ID: <Jan70@hoge.baba.hajime.jp>
Mime-Version: 1.0
Content-Type: TEXT/PLAIN; charset=US-ASCII
Status: R


Dear Dr. Kato,

Please encourage your observers to watch PG 0943+521, since a definitive
orbital period still is needed: the spectroscopic period I found for my
thesis was probably my worst ever. 

Best, Fred

=====================================
On Sun, 9 Jan 1994, Taichi Kato wrote:

>   (2) PG 0943+521
> 
>    Cataclysmic varibale PG 0943+521 is currently experiencing a plateau
>    following an outburst, just like standstills in some Z Cam stars
>    (G. Poyner, private communication).
>    A series of V-band CCD photometry has revealed periodic modulation
>    with a period of 0.0655 day (or its one-day aliases) and an amplitude
>    of 0.15 mag.  The light curve shows rather sharp minimum in contrast
>    to usual superhumps in SU UMa stars, but the short period and the
>    constancy of the profile support the idea that the object really
>    belongs to the SU UMa subclass.  Further observations are recommended
>    to follow its outburst behavior.
> 
>    The object is located at 09h 43m 50.75s +52deg 08' 03.6" (J1950.0)

===========================================================================
Fred Ringwald                        ... to further the progress of science,
Department of Physics                    to guide to an understanding 
Keele University, Keele                       of the majesty of the heavens,
Staffordshire, ST5 5BG                   to emphasize that 
England                                 under the great celestial firmament,
                                 there is order, interdependence, and unity.
Internet: far@astro.keele.ac.uk               -- Adler Planetarium, Chicago  
JANET: FAR@UK.AC.KEELE.PHYSICS.STARLINK 
DECnet: KLVAD::FAR   Phone: +44-0782-621111 ext. 7892  Fax: +44-0782-711093

>From ALEX@BKYAST.BERKELEY.EDU Mon Jan 10 03:54:11 1994
Date:    Sun, 9 Jan 1994 10:49:33 -0800 (PST)
From: ALEX@BKYAST.BERKELEY.EDU (ALEX FILIPPENKO, UC BERKELEY, 510-642-1813)
Message-ID: <Jan70@hoge.baba.hajime.jp>
Subject: J0422+32
To: rmw@altair.lowell.edu, tkato@kusastro.kyoto-u.ac.jp
X-Vmsmail-To: SMTP%"rmw@altair.lowell.edu", SMTP%"tkato@kusastro.kyoto-u.ac.jp"
Status: R

  Mark and/or Taichi,
  Could you help Dr. Munari get a finding chart and the comparison 
sequence? Thanks.
   Alex
***
From:	SMTP%"munari@astrpd.DNET.NASA.GOV"  9-JAN-1994 06:05:31.35
To:	"alex@bkyast.berkeley.edu"@6913.DNET.NASA.GOV
Subj:	RE: GRO J0422+32

Dear Alex,
   I could join the observing effort on GRO J0422+32 with low resolution
330-1100 nm CCD spectrophotometry, 450-700 high resolution CCD echelle
spectra as well as photographic photometry (BVI bands) or CCD photometry.
What I need is a usable finding chart. I understand that a comparison
sequence is available too.
  Could you Fax them both me at Asiago ? I'm going to have observing time
at the 1.8 m telescope in coming days and weeks.
Thanks and a happy new year. 
Ulisse Munari (fax +39-424-462884)
******************************
   1-9-94
Ulisse,
   I don't have a finding chart handy of GRO J0422+32 (I know what the
field looks like when I go to the telescope), but I will pass your
message on to Mark Wagner and Taichi Kato. Perhaps they could help.
   Good luck!
   Alex
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