… In addition to the above, 20 to 25 more uncertain members are known, some of which are shown in parentheses in the figure. Of these, Maffei 1 and 2 were discovered by P. Maffei in 1968. Although both are fairly bright galaxies, they are hidden by dense interstellar dust because they are in the constellation Cassiopeia, close to the galactic plane. He was the first to detect them using near-infrared photography. … *Some of the terminology that mentions "Maffei, P." is listed below. Source | Heibonsha World Encyclopedia 2nd Edition | Information |
… 以上のほか,やや不確定なメンバーが,20~25個知られており,図の中でかっこをつけて示したのはその一部である。このうちマフェイ1と2は,1968年マフェイP.Maffeiが見つけたもので,どちらもかなり明るい銀河であるのに,銀河面に近いカシオペヤ座にあるため,濃い星間塵に隠されていた。彼は近赤外写真によって,これらを初めて検出したのである。… ※「Maffei,P.」について言及している用語解説の一部を掲載しています。 出典|株式会社平凡社世界大百科事典 第2版について | 情報 |
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