[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-id 748] Re: [vsnet-newvar 1835] Variables in the field of V1413 Aql
- Date: Mon, 17 Feb 2003 12:13:28 -0700 (MST)
- To: tkato@kusastro.kyoto-u.ac.jp
- From: Brian Skiff <Brian.Skiff@lowell.edu>
- Subject: [vsnet-id 748] Re: [vsnet-newvar 1835] Variables in the field of V1413 Aql
- Cc: vsnet-id@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-id-archive@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-id@ooruri.kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-id@ooruri.kusastro.kyoto-u.ac.jp
>> Amplitudes are 0.34, 0.51 and 0.64 mag in the
>> VRI bands, respectively.
Are the amplitudes reversed? One would expect the amplitudes for
red stars to decline toward the red. If the numbers are correct (larger
amplitude at I compared to V), then I would immediately worry about the
validity of the results.
'Best' position for this star, by the way, is from the Bordeaux
meridian circle: 19 03 33.40 +16 31 19.6 (J2000).
\Brian
Return to Home Page
Return to the Powerful Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
Powered by ooruri technology