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<blockquote data-quote="tmjuju" data-source="post: 614942" data-attributes="member: 2204"><p>Λίγο πιο hard-core…</p><p>Ένα ανεξήγητο ακόμα φαινόμενο που παρατηρήθηκε. </p><p>Here we report the observations of the optical transient</p><p>SCP 06F6 discovered during the course of the 2005-2006</p><p>Hubble Space Telescope (HST) Cluster SN Survey (PI:</p><p>Perlmutter; Dawson et al. 2008, in preparation). The</p><p>discovery was originally reported in a June 2006 IAU</p><p>circular (Dawson et al. 2006). Its lightcurve rise time of</p><p>_100 days is inconsistent with all known SN types, and</p><p>its spectroscopic attributes are not readily matched to</p><p>any known variable. We present photometry in §2 and</p><p>spectroscopy in §3. In §4, we discuss constraints and</p><p>summarize.</p><p></p><p><a href="http://arxiv.org/PS_cache/arxiv/pdf/0809/0809.1648v1.pdf" target="_blank">http://arxiv.org/PS_cache/arxiv/pdf/0809/0809.1648v1.pdf</a></p><p></p><p>(pdf ~500Kb)</p></blockquote><p></p>
[QUOTE="tmjuju, post: 614942, member: 2204"] Λίγο πιο hard-core… Ένα ανεξήγητο ακόμα φαινόμενο που παρατηρήθηκε. Here we report the observations of the optical transient SCP 06F6 discovered during the course of the 2005-2006 Hubble Space Telescope (HST) Cluster SN Survey (PI: Perlmutter; Dawson et al. 2008, in preparation). The discovery was originally reported in a June 2006 IAU circular (Dawson et al. 2006). Its lightcurve rise time of _100 days is inconsistent with all known SN types, and its spectroscopic attributes are not readily matched to any known variable. We present photometry in §2 and spectroscopy in §3. In §4, we discuss constraints and summarize. [url]http://arxiv.org/PS_cache/arxiv/pdf/0809/0809.1648v1.pdf[/url] (pdf ~500Kb) [/QUOTE]
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