1983
DOI: 10.1007/bf01005668
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On markaryan 6 and the problem of the intermediate Sy 1.5 type

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“…Pension and Perez (1984) saw a very clear and spectacular change in the continuum and BLR of the most famous Seyfert, NGC 4151, and advanced the idea that Seyferts could change types on a very fast time scale (decades). Changes from Type 2 to Type 1 have also been seen in Mkn 6 by Khachikian, Popov, and Egiazaryan (1982) and in NGC 1566 by Alloin et al (1984). Even without a starburst fossil, as in the Adams and Weedman idea, the NLR would remain essentially unchanged over such time scales because of its large size.…”
Section: Hi Some General Pointsmentioning
confidence: 95%
“…Pension and Perez (1984) saw a very clear and spectacular change in the continuum and BLR of the most famous Seyfert, NGC 4151, and advanced the idea that Seyferts could change types on a very fast time scale (decades). Changes from Type 2 to Type 1 have also been seen in Mkn 6 by Khachikian, Popov, and Egiazaryan (1982) and in NGC 1566 by Alloin et al (1984). Even without a starburst fossil, as in the Adams and Weedman idea, the NLR would remain essentially unchanged over such time scales because of its large size.…”
Section: Hi Some General Pointsmentioning
confidence: 95%