[Date Prev][Date Next][Thread Prev][Thread Next][Date Index][Thread Index]

Re: NSV 10892

To: "Dirk Terrell" <terrell@boulder.swri.edu>
Subject: Re: NSV 10892
From: Michael Koppelman <lolife@bitstream.net>
Date: Fri, 9 Aug 2002 16:50:50 -0500
Cc: "TASS" <tass@listserv.wwa.com>
In-Reply-To: <200208091625.g79GP1K28813@perseus.boulder.swri.edu>
Sender: owner-tass@listserv.wwa.com

On Friday, August 9, 2002, at 11:25  AM, Dirk Terrell wrote:

> This one will be tough for two reasons: (1) it has a large O-Connell
> effect (maxima at different levels) indicating spot or other activity
> and (2) the eclipses are partial so you will have almost no handle on
> the mass ratio.

Don't get me wrong: I don't know an eclipse model from a hole in the 
ground, but I played with the Wilson-Devinney code and came up with this:

http://www.lolife.com/astronomy/gsc445-1993/model.jpg

If I knew how to bring down the second maximum, I think it would tuck into 
place. I don't know if it is a physically possible solution or not.

Michael K.

References:
- Re: NSV 10892
  - From: "Dirk Terrell" <terrell@boulder.swri.edu>

Prev by Date: Re: Modified WS
Next by Date: Re: Tass reference catalog
Prev by thread: Re: NSV 10892 - not a cluster member
Next by thread: RE: NSV 10892
Index(es):
- Date
- Thread