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[vsnet-chat 5591] BD+59 224 V, Rc, and H alpha Photometry
- Date: Tue, 22 Oct 2002 07:05:24 EDT
- To: Brian.Skiff@lowell.edu
- From: DWest61506@aol.com
- Subject: [vsnet-chat 5591] BD+59 224 V, Rc, and H alpha Photometry
- Cc: vsnet-chat@kusastro.kyoto-u.ac.jp, aavso-discussion@informer2.cis.mcmaster.ca
- Delivered-To: vsnet-chat@kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp
Brian:
I have made some additional measurements of BD+59 224 (see below). From my observations I can conclude two things: 1. Variability is small over the past three weeks. 2. H alpha emission is present. Non-emission line stars have H alpha ~2. An H alpha of 1.89 indicates weak H alpha emission. Does the presence of H alpha emission provide more evidence supporting the possibility that this is a VV Cep type of system?
Regards,
Doug West
http://hometown.aol.com/dwest61506/index.html
Photometry (without color correction)
Star UT Date/Time Measurements
BD+59 224 10/21/2002 01:32 V=9.39
GSC 4030:591 10/21/2002 01:32 V=10.20
BD+59 224 10/22/2002 01:28 V=9.38
GSC 4030:591 10/22/2002 01:28 V=10.19
BD+59 224 10/22/2002 01:32 Rc=8.42
GSC 4030:591 10/22/2002 01:32 Rc=10.06
BD+59 224 10/22/2002 01:35 H alpha = 1.89 +/-0.01
GSC 4030:591 10/22/2002 01:35 H alpha = 2.02 +/-0.02
Previous Photometry (without color transformation) 09/29/2002 2:21UT:
GSC 4030:591 V=10.28 +/-0.06, B-V= -0.06+/-0.15, V-Rc=0.23+/-0.07
BD+59 224 V= 9.38 +/-0.06, B-V= 1.31+/-0.15, V-Rc=0.97+/-0.07
Comparison stars for photometry:
GSC 4030:427 [BD+59 227] B=11.57, V=10.48, Rc=9.88
SAO 11690 [HD 7796] B=9.59, V=9.47, Rc=9.39
B&V from Tycho 1, Rc from conversion formula at: http://hometown.aol.com/dwest61506/page32.html
Information on H alpha photometry:
http://members.aol.com/dwest61506/page34.html
http://hometown.aol.com/dwest61506/page35.html
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