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“…Note that it is coherent with ground based observations obtained at the same epoch (see R. Cumming cited in Plait et al 1995) giving a ring intensity of 15 10 −14 erg s −1 cm −2 . In addition, the flux of the central star obtained with IDEA is compatible with a unique decay rate between days 1275 and 2522 (see Jakobsen et al 1994). The profile of the central star of the supernova presented in Sect.…”
Section: Sn 1987asupporting
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“…Note that it is coherent with ground based observations obtained at the same epoch (see R. Cumming cited in Plait et al 1995) giving a ring intensity of 15 10 −14 erg s −1 cm −2 . In addition, the flux of the central star obtained with IDEA is compatible with a unique decay rate between days 1275 and 2522 (see Jakobsen et al 1994). The profile of the central star of the supernova presented in Sect.…”
Section: Sn 1987asupporting
“…The IDEA solution is close to the RLM deconvolution of Plait et al (1995) (applied to a higher signal-to-noise ratio image). The IDEA image is also similar to the COSTAR-corrected images presented by Jakobsen et al (1994) even though the ring structure might have evolved between the two epochs.…”
Section: Sn 1987asupporting
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“…Jakobsen et al (1991) demonstrated that the expanding envelope of SN 1987A was spatially resolved by HST already in the first FOC images taken 1278 days after the explosion. These data combined with subsequent FOC observations made on days 1754, 2511 and 2533 showed that the outer envelope of SN 1987A was expanding linearly with time in a self-similar fashion (Jakobsen et al 1994).…”
Section: Introductionmentioning
“…Subsequent observations made with the FOC allowed Jakobsen et al [24,25] to measure the angular expansion of the supernova ejecta. The results confirmed the validity of the expansion models put forward on the basis of spectroscopy.…”
Section: Hst Observationsmentioning