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《Planetary and Space Science》2007,55(4):532-533
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Jian-Jun Zhou Xi-Zheng Zhang Hong-Bo Zhang Jarken Esimbek Ju-Yong Zhang Bing-Gang Ju 《中国天文和天体物理学报》2007,7(5):705-711
We made the first CO(I—0) mapping to SNR G21.8-0.6 and SNR G32.8-0.1, both associated with OH 1720 MHz maser.Based on the morphological correspondence and velocity and position agreement between the radio remnant and the CO clouds,we tentatively identify the clouds that are respectively interacting with the two SNRs. 相似文献
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Ham-Erich Frohlich 《Astronomische Nachrichten》1989,310(3):248-249
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Hans-Jürgen Schmidt 《Astronomische Nachrichten》1987,308(1):62-62
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Johann Dorschner 《Astronomische Nachrichten》1990,311(4):262-262
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