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[vsnet-campaign-sn 482] spectral type of recent SNe
Dear SN watchers,
IAUC 7979 informed the spectral classification of two SNe.
SN 2002fi:
In [vsnet-obs 41399]: (Sept. 18)
>SN2002fi 20020828.4 <190:C KAI
>SN2002fi 20020913.4 185:C KAI
>SN2002fi 20020917.4 183:C KAI
>
># MCG -04-7-10, a host galaxy of SN 2002fi, is a distant spiral
># ((R'?)SA(s)a) galaxy. The reported magnitude is coincident with
># the expected maximum for typical SN Ia.
It was indeed of type Ia. Features resembles that of 20 days after
maximum on Sept. 26.
SN 2002fj:
In [vsnet-campaign-sn 475]: (Sept. 20)
># NGC 2642, a host galaxy of SN 2002fj, is a barred-spiral (SB(r)bc)
># galaxy in a dawn sky. SN is located at the east end of the bar, and
># just south of a foreground star (mag 13). The expected maximum for
># typical SN Ia is mag about 15.5. The reported fast decline is quite
># exceptional for SNe, so follow-up photometry and spectroscopy is
># very urged.
It was revealed to be type IIn SN. Rapid decline would be consistent
with this classification. Recent magnitude estimate is:
>SN2002fj 020928.122 170CR MLF
Sincerely Yours,
Hitoshi Yamaoka, Kyushu Univ., Japan
yamaoka@rc.kyushu-u.ac.jp
Return to Daisaku Nogami
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