Beobachtung der Nova Persei (Ch. 1226)
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چکیده
منابع مشابه
A multiwavelength study of the remnant of nova GK Persei
We present new observations of the nebular remnant of the old nova GK Persei 1901, in the optical using the Himalayan Chandra Telescope (HCT) and at low radio frequencies using the Giant Metrewave Radio Telescope (GMRT). The previous such study was by Seaquist et al (1989, hereafter S89). The dimensions of the shell in the optical emission lines of [NII], [OIII] and [OII] are 108×94 arcsec, 104...
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ژورنال
عنوان ژورنال: Astronomische Nachrichten
سال: 1903
ISSN: 0004-6337,1521-3994
DOI: 10.1002/asna.19031612207