RADIOASTRONOMICAL OBSERVATIONS OF COMETS IRAS-ARAKI-ALCOCK (1983D) AND SUGANO-SAIGUSA-FUJIKAWA (1983E)

RADIOASTRONOMICAL OBSERVATIONS OF COMETS IRAS-ARAKI-ALCOCK (1983D) AND SUGANO-SAIGUSA-FUJIKAWA (1983E)
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DOI：
10.1016/0019-1035(84)90150-7
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发表时间：
1984-10
期刊：
Icarus
影响因子：
3.2
通讯作者：
W. Irvine;Z. Abraham;M. A’Hearn;W. Altenhoff;C. Andersson;J. Bally;W. Batrla;A. Baudry;D. Bockelée-Morvan;G. Chin;J. Crovisier;I. Pater;D. Despois;L. Ekelund;É. Gérard;T. Hasegawa;C. Heiles;J. Hollis;W. Huchtmeier;N. Kaifu;R. Levreault;C. Masson;P. Palmer;M. Pérault;L. Rickard;A. Sargent;E. Scalise;F. Schloerb;J. Schmidt;A. Stark;M. Stevens;P. Stumpff;E. Sutton;D. Swade;M. Sykes;B. Turner;C. Wade;M. Walmsley;J. Webber;A. Winnberg;A. Wootten
W. Irvine;Z. Abraham;M. A’Hearn;W. Altenhoff;C. Andersson;J. Bally;W. Batrla;A. Baudry;D. Bockelée-Morvan;G. Chin;J. Crovisier;I. Pater;D. Despois;L. Ekelund;É. Gérard;T. Hasegawa;C. Heiles;J. Hollis;W. Huchtmeier;N. Kaifu;R. Levreault;C. Masson;P. Palmer;M. Pérault;L. Rickard;A. Sargent;E. Scalise;F. Schloerb;J. Schmidt;A. Stark;M. Stevens;P. Stumpff;E. Sutton;D. Swade;M. Sykes;B. Turner;C. Wade;M. Walmsley;J. Webber;A. Winnberg;A. Wootten
中科院分区：
物理与天体物理2区
文献类型：
--
作者：
W. Irvine;Z. Abraham;M. A’Hearn;W. Altenhoff;C. Andersson;J. Bally;W. Batrla;A. Baudry;D. Bockelée-Morvan;G. Chin;J. Crovisier;I. Pater;D. Despois;L. Ekelund;É. Gérard;T. Hasegawa;C. Heiles;J. Hollis;W. Huchtmeier;N. Kaifu;R. Levreault;C. Masson;P. Palmer;M. Pérault;L. Rickard;A. Sargent;E. Scalise;F. Schloerb;J. Schmidt;A. Stark;M. Stevens;P. Stumpff;E. Sutton;D. Swade;M. Sykes;B. Turner;C. Wade;M. Walmsley;J. Webber;A. Winnberg;A. Wootten

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1983d 和 1983e 彗星的射电观测报告了连续发射（1 ≤ λ ≤6 cm）和谱线发射（OH、CO、CS、HCN、HCO+、CN、CH3CN、CH3C2H、NH3、H2O、HC3N、CH3CH2CN）的检测和上限。与光波长下 CN 的观测结果进行了比较。这些结果可能有助于规划未来的彗星观测。
Detections and upper limits to the continuum emission (1 ≤ λ ≤6 cm) and spectral line emission (OH, CO, CS, HCN, HCO+, CN, CH3CN, CH3C2H, NH3, H2O, HC3N, CH3CH2CN) are reported from radio observations of Comets 1983d and 1983e. Comparison is made with observations of CN at optical wavelengths. These results may be useful in planning future cometary observations.