Evidence for weak maser action in interstellar cyanodiacetylene
The J=1..-->..0 and J=8..-->..7 rotational transitions of interstellar cyanodiacetylene have been observed in Sgr B2. These observations confirm the earlier detection of this heavy molecule, and provide further information on its excitation. The J=8..-->..7 line and the previously observed...
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Veröffentlicht in: | Astrophys. J., Lett.; (United States) Lett.; (United States), 1976-11, Vol.209, p.L143 |
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Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | The J=1..-->..0 and J=8..-->..7 rotational transitions of interstellar cyanodiacetylene have been observed in Sgr B2. These observations confirm the earlier detection of this heavy molecule, and provide further information on its excitation. The J=8..-->..7 line and the previously observed J=4..-->..3 line can be fitted to a thermal equilibrium model and give a total column density of 1.5 x 10/sup 14/ cm/sup -2/. The J=1..-->..0 transition is much stronger than expected from thermal equilibrium, and suggests maser action. (AIP) |
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ISSN: | 0004-637X 1538-4357 |
DOI: | 10.1086/182285 |