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Дата изменения: Unknown Дата индексирования: Sat Dec 22 06:53:36 2007 Кодировка: Поисковые слова: viking 2 |
Supernova 2002bx in IC 2461
This page is devoted to information on Supernova 2002bx in IC 2461 Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page.  Information on the original web pages for many of these images can be found on the updates and links web pages.
Discovered independantly by
LOTOSS and
Tom Boles (UK).
This is found to be a type II supernova on the rise in an edge on galaxy.
We have a DSS Photometry reference image made by Odd Trondal. 
Icon generated from the Pollux Observatory image.
The following is a list of images of this SN, in chronological order. Click on the name in the "observer" column to see the image. Times and dates are in UT unless otherwise noted. If you know of any others, please tell me!
Image Credit | Date | Mag | Filter | Comments |
---|---|---|---|---|
LOTOSS image | 2002/04/01.2 | 16.8 | C | Discovery |
Tom Boles image | 2002/04/01.943 | 16.2 | C | Discovery, mirror, local mirror |
Mark Armstrong image | 2002/04/03.900 | C | ||
G. Vandenbulcke image | 2002/04/04 | C | ||
Remanzacco Obs image | 2002/04/04 | C | ||
A. Leroy image | 2002/04/04.918 | CR | ||
Fred Ewalt image | 2002/04/05.076 | 16.7 | C | |
Matin Mobberley image | 2002/04/05.852 | C | ||
J.B. De Vanssay image | 2002/04/08.907 | 16.4 | CR | |
R. Poncy image | 2002/04/09.821 | 16.7 | CR | |
Pepe Manteca image | 2002/04/09.989 | 16.7 | CR | |
Diego Rodriguez image | 2002/04/09.989 | 16.7 | CR | |
Fred Ewalt | 2002/04/11.055 | 16.6 | C | color version |
Rafael Ferrando image | 2002/04/13.840 | 16.37 | CR | |
Esteban Reina Lorenz image | 2002/04/13.889 | 16.25 | CR | |
Josch Hambsch image | 2002/04/13.903 | 16.6 | C | |
Arnaud Leroy image | 2002/04/13.969 | 16.5 | CR | |
Pedro Re' image | 2002/04/15.890 | 16.29 | C | |
Rafael Ferrando image | 2002/04/15.890 | 16.41 | CR | |
Rui Goncalves image | 2002/04/15.958 | 16.1 | CR | |
R. Poncy image | 2002/04/16.871 | 16.6 | CR | |
Pepe Manteca image | 2002/04/17.900 | 16.42 | CR | |
James R. Foster image | 2002/04/18.187 | LRGB | ||
Diego Rodriguez image | 2002/04/23.910 | 16.45 | CR | |
Eric Barbotin image | 2002/04/24.878 | 16.5 | CR | |
J.B. De Vanssay image | 2002/04/24.930 | 16.4 | CR | |
JM Llapasset image | 2002/04/30.840 | 16.4 | CR | |
Albert Sanchez image | 2002/04/30.871 | 16.47 | V | |
Rafael Ferrando image | 2002/04/30.881 | 16.4 | CR | |
Kopernik image | 2002/05/04.212 | 16.58 | C | |
Rafael Ferrando image | 2002/05/04.836 | 16.4 | CR | |
Rezman Obs image | 2002/05/06.837 | C | ||
Rafael Ferrando image | 2002/05/11.891 | 16.46 | CR | |
R. Poncy image | 2002/05/12.853 | 16.6 | CR | |
JM Llapasset image | 2002/05/14.867 | 16.2 | CR | |
JB DeVanssay image | 2002/05/15.921 | 16.4 | CR | |
J Nicolas image | 2002/05/16.852 | 16.2 | CR | |
Rafael Ferrando image | 2002/05/17.839 | 16.42 | CR | |
Pepe Manteca | 2002/05/19 | 16.57 | R | |
A. Leroy image | 2002/05/20.881 | 16.5 | CR | |
Rafael Ferrando image | 2002/05/24.900 | 16.4 | CR | |
Albert Sanchez image | 2002/05/30.890 | 16.4 | C | |
J Nicolas image | 2002/05/31.878 | 16.7: | CR | |
Rafael Ferrando image | 2002/06/02.876 | 16.44 | CR | |
Rafael Ferrando image | 2002/06/08.899 | 16.58 | CR |
Dear SN watchers,
The KAIT team and Tom Boles has discovered a probably rising nearby SN in the galaxy on the border of Lyn-LMi. The expected maximum for typical SN Ia is mag about 14.0.
SN 2002bx is discovered by the KAIT team on Mar 31.2 at mag about 16.9, and confirmed on the next night (mag 16.8). Tom independently discovered it on Apr. 1.943, when he estimated the magnitude as 16.2. The position of the new object (the KAIT measurement) is: R.A. = 9h19m54s.98, Decl. = +37o12'08".3 (2000.0), which is about 37" west and 40" north of the nucleus of the edge-on spiral (Sbc) galaxy IC 2461. The SN is almost superimposed on, but slightly (2-3") south of, the disk plane. No confusing foreground star are there. Several mag 15 stars are around the galaxy, but because of their redness, take care in choosing the comparison stars in the magnitude estimates.
The recession velocity of IC 2461 is measured as 2260 km/s. The Galactic extinction is negligible. If it is unreddened by the interstellar matter in the host galaxy, the expected maximum for typical SN Ia is mag about 14.0. The spectroscopic classification and the followup magnitude estimates are urged.
Sincerely Yours,
Hitoshi Yamaoka, Kyushu Univ., Japan
yamaoka@rc.kyushu-u.ac.jp
SN2002bx 20020311.2 <185:C KAI SN2002bx 20020331.2 169:C KAI SN2002bx 20020401.2 168:C KAI SN2002bx 20020401.943 162C Bol
The host galaxy of SN 2002bx is IC 2461, a somewhat nearby edge-on spiral galaxy. The expected maximum for SN Ia is mag about 14.0. The information will be posted on vsnet-campaign-sn.
In [vsnet-campaign-sn 397]:
It is normal type-II SN caught on the early phase. The continuum is quite blue, but narrow Na D lines are visible.
The spectra of these supernovae can be seen at the CfA site: http://cfa-www.harvard.edu/supernova/RecentSN.html .