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[vsolj-alert 306] SN1999by sequence update (Skiff)
- Date: Sun, 2 May 1999 12:30:18 +0900 (JST)
- To: vsolj-alert@ooruri.kusastro.kyoto-u.ac.jp
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsolj-alert 306] SN1999by sequence update (Skiff)
- Sender: owner-vsolj-alert@ooruri.kusastro.kyoto-u.ac.jp
From owner-vsnet-alert@kusastro.kyoto-u.ac.jp Sun May 2 12:18 JST 1999
Date: Sat, 1 May 1999 20:20:13 -0700
From: bas@lowell.Lowell.Edu (Brian Skiff)
To: aavso-discussion@physics.mcmaster.ca, vsnet-alert@kusastro.kyoto-u.ac.jp,
vsnet-chart@kusastro.kyoto-u.ac.jp
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Subject: [vsnet-alert 2919] Another star for NGC 2841 sequence
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While looking in the literature to see if there was additional data for
stars in the field of NGC 2841, I found a paper by Tsvetkov (1986 Perem. Zvezdy
22, 279) that shows additional photoelectric photometry for some bright stars
in the field. There appears to be a zero-point offset in his data when
compared to both Hipparcos data and the BVRI data I gave originally (which is
from unpublished results by Corwin and Frueh). One of the stars is suitably
placed both fairly near the galaxy and in the right magnitude range. I give
this star below in the amended table (star "3Ts"). I have adjusted the V
magnitude by +0.08 and the B-V color by +0.03 to bring it in line with the
other stars. The V-R color in parens is derived from the B-V color.
For CCD observers desiring R magnitudes, simply _subtract_ V-R from V to
get R magnitudes explicitly.
\Brian
Name RA (2000) Dec s GSC V B-V V-R V-I
NGC 2841 1 9 22 28.4 +51 00 51 G 3431-0219 8.48 1.29 0.67 1.23
NGC 2841 2 9 21 50.8 +51 00 36 G 3431-0625 11.07 0.59 0.33 0.65
NGC 2841 3Ts 9 22 34.9 +51 04 13 G 3431-0388 12.62 0.64 (0.37)
NGC 2841 3 9 21 47.3 +50 58 50 G 3431-0053 13.51 0.75 0.43 0.83
NGC 2841 4 9 21 58.2 +51 00 16 G 3431-0495 13.77 0.60 0.40 0.74
NGC 2841 5 9 22 02.3 +51 01 23 G 3431-0159 14.19 0.83 0.42 0.91
NGC 2841 147 9 22 06.8 +50 53 37 G 3431-0802 14.72 0.88
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