A search for 1404-MHz H-2(+) line emission in the atmosphere of Jupiter and the radio source Sgr B2

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作者
Venger, AP
Gosachinskii, IV
Dubrovich, VK
Lipovka, AA
Morozov, AS
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P1 [天文学];
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0704 ;
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Measurements of the spectrum of Jupiter and the radio source Sgr B2 in the 1404.49-MHz line for the superfine transition (G'G'-GF) = 3/2, 5/2-1/2, 3/2 of the molecular ion H-2(+) are observed at the 4 sigma level. Various models that could lead to a significant abundance of H-2(+) are discussed. Expected brightness temperatures are estimated.
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页码:370 / 372
页数:3
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