2006CBET..506....1B

Query : 2006CBET..506....1B

2006CBET..506....1B - Central Bureau Electronic Telegrams, 506, 1 (2006/May-0)

Supernova 2006cc in UGC 10244.

BLONDIN S., MODJAZ M., KIRSHNER R., CHALLIS P. and PETERS W.

Abstract (from CDS):

S. Blondin, M. Modjaz, R. Kirshner, and P. Challis, Harvard-Smithsonian Center for Astrophysics, report that a spectrum (range 350-740 nm) of SN 2006cc (cf. CBET 505), obtained on May 8.34 UT by W. Peters with the F. L. Whipple Observatory 1.5-m telescope (+ FAST), shows it to be a reddened type-Ia supernova around maximum light. Cross-correlation with a library of type-Ia supernova spectra indicates that SN 2006cc is most similar to the 1991T-like SN 1998es (cf. IAUC 7054) at 1 day past maximum. A comparison plot can be seen at the following URL: http://cfa-www.harvard.edu/oir/Research/ supernova/spectra/sn2006cc_comp.gif Adopting a recession velocity of 9777 km/s for the host galaxy (from "The Updated Zwicky Catalog", http://tdc-www.harvard.edu/uzc/), the maximum absorption in the relatively weak Si II line (rest 635.5 nm) is blueshifted by roughly 12000 km/s. Also, interstellar Na I D absorption at the redshift of the host galaxy is visible in the spectrum with an equivalent width of 0.3 nm.

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Journal keyword(s):

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 SN 2006cc SN* 16 09 56.470 +43 07 35.90     18.3     SNIa 36 1

Query : 2006CBET..506....1B

Basic data :
SN 2006cc -- SuperNova
Other object types: otypes_help 		SN* (2012MNRAS,SN)
ICRS coord. (ep=J2000) : 		16 09 56.470 +43 07 35.90 (Optical) [ ] D 2022PASA...39...46C
FK4 coord. (ep=B1950 eq=1950) : 		16 08 18.213 +43 15 21.94 [ ]
Gal coord. (ep=J2000) : 		068.173324 +47.094860 [ ]
Radial velocity / Redshift / cz : 		V(km/s) 9672 [~] / z(~) 0.0328 [~] / cz 9833 [~]
   D 2010ApJ...715..743K
Spectral type: 		SNIa C 2008yCat....1.2024B
Fluxes (1) :
V 18.3 [~] D 2008yCat.2283....0B
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SN 2006cc

References (36 between 1850 and 2026) (Total 36)
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