Issue |
A&A
Volume 545, September 2012
|
|
---|---|---|
Article Number | L7 | |
Number of page(s) | 8 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361/201220105 | |
Published online | 13 September 2012 |
Online material
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Fig. 4
(Top-left panels) Na i D absorption features in the high resolution spectrum of SN 2008J. Several components are present and their peak positions are indicated by black solid lines. The features are fit with the sum of 9 Gaussian functions, the best fit is shown in red. Velocity is plotted in the SN rest frame, as determined from the narrow emission line peaks in the same high resolution spectrum. (Bottom-left panels) Hα and Hβ sequences from the low resolution spectra, shown after low-order polynomial continuum subtraction. Each profile is well fit by the sum (in red) of two Lorentzian components (in blue and green). (Right panels) Narrow emission lines in the high-resolution spectrum of SN 2008J. Each line has been fit with a Lorentzian profile for the emission and one for the absorption when detected. The absorption component is shown in blue, the total best fit in red. The spectrum is presented in velocity scale, where the zero velocity corresponds to the emission peak position. |
Open with DEXTER |
Optical and near-infrared photometry of the local sequences in the standard system.
Optical photometry of SN 2008J in the natural system.
NIR photometry of SN 2008J in the natural system.
Spectroscopic observations of SN 2008J.
Parameters from the narrow emission line fit.
Peak magnitudes of SN 2008J.
© ESO, 2012
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