Spectroscopic observations of SN1987a in the LMC |
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Authors: | J B Hearnshaw V J McIntyre A C Gilmore |
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Institution: | (1) Mt John University Observatory and Department of Physics, University of Canterbury, Private Bag, Christchurch, New Zealand |
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Abstract: | This paper describes the results of optical spectroscopy of SN1987a carried out at Mt John University Observatory on a regular
basis since 1987 February 25. Typical spectra are presented in an evolutionary sequence, and velocities of Balmer and selected
metallic lines are measured in either emission or absorption. The velocities are interpreted together with the results of
photoelectric photometry. The Barnes-Evans relationship has been applied to the photometry to give an angular diameter of
the photosphere. The expansion velocity of the photosphere is initially about 3700 km s-1 which is similar to the asymptotic value from weaker absorption lines such as the MgIb line. After 40 days the photosphere
appears to expand more slowly and it reaches a maximum size of about 145 A.U. after about 100 days before receding inwards.
The photometry and spectroscopy together result in a distance modulus of 18.3 ± 0.2. |
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Keywords: | Supernovae SN1987a optical spectra |
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