[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]

[vsnet-chat 6210] Bright miras and lightcurves




----- Original Message -----
From: Stan Walker
To: vsnet-chat@kusastro.kyoto-u.ac.jp
Sent: Tuesday, April 08, 2003 4:40 PM
Subject: [vsnet-chat 6206] R Carinae


>>> One of the target stars will be R Carinae and I notice it's bright at
the moment. But is it rising or falling - can anyone comment? What's the
state of any other bright Miras?

Hi, Stan:

We are lucky to have this very bright star in one of its brightest maxima
right now!
It is rising around 4.5 but it's more than a month before its predicted
maximum, so it will probably be one of its brightest performances (its
brigthest recorded maximum is 3.9 according to the GCVS).
The last 4 or 5 days the rising trend has slowed down so we have to watch
before speaking.

S Carinae is in a very interesting maximum around 6.2, since it showed a
hump in the ascending branch a couple of weeks ago.

R Hydrae is also rising and although it's been around ten days I don't
observe it, I can tell it is around 6.5-7.0 magnitude.

R Centauri is past minimum (at 8.2) and have started its way to secondary
maximum (now 8.0).

BH Crucis is also rising. After a secondary maximum at 7.3 and a drop to 7.4
is now rising faster and getting to 7.0. A very good moment to observe this
very red mira star. As R Cen its period is changing. It lenghtend from 419
days (1973) to 550 days (now)

I am uploading my more recent lightcurves for bright miras right now, so
take a look!

http://ar.geocities.com/varsao/Curva_R_Car.htm
http://ar.geocities.com/varsao/Curva_S_Car.htm
http://ar.geocities.com/varsao/Curva_R_Hya.htm
http://ar.geocities.com/varsao/Curva_R_Cen.htm
http://ar.geocities.com/varsao/curva_BH_Cru.htm

There are also updated lightcurves for eta Carinae (slowly brightening) and
theta Apodis (beautiful!).

http://ar.geocities.com/varsao/Curva_Eta_Carinae.htm
http://ar.geocities.com/varsao/Curva_The_Aps.htm

Regards,
Sebastian.






Return to Home Page

Return to the Powerful Daisaku Nogami

vsnet-adm@kusastro.kyoto-u.ac.jp

Powered by ooruri technology