彗星C/2002 T7的光谱(LINEAR)

IF 0.2 Q4 ASTRONOMY & ASTROPHYSICS Advances in Astronomy and Space Physics Pub Date : 2020-01-01 DOI:10.17721/2227-1481.10.43-47
O. Shubina, N. Borisov, V. Rosenbush, O. Ivanova
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摘要

本文介绍了在俄罗斯特殊天体物理天文台1米蔡司-1000望远镜上对彗星C/2002 T7 (LINEAR)进行的光谱观测结果。光谱是在2003年11月13日、14日和21日彗星经过近日点之前,在3500-7500 Å波长范围内获得的,当时彗星的日心距离和地心距离分别约为2.7 AU和1.8 AU。光谱没有显示出CN, C2和C3分子的最强彗星发射的任何发射特征。11月14日和21日反射率的归一化光谱梯度分别为2.8% / 1000 Å和5.4% / 1000 Å。表征彗星尘埃产生率的Afρ参数平均约为800厘米。彗星C/2002 T7 (LINEAR)可以被归类为尘埃彗星
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Spectra of comet C/2002 T7 (LINEAR)
We present the results of spectral observations of comet C/2002 T7 (LINEAR) carried out at the 1-m Zeiss-1000 telescope of the Special Astrophysical Observatory (Russia). The spectra were obtained within the 3500-7500 Å wavelength range on November 13, 14, and 21, 2003, before the perihelion passage, when heliocentric and geocentric distances of the comet were about 2.7 AU and 1.8 AU, respectively. Spectra do not show any emission features from the strongest cometary emissions of the CN, C2, and C3 molecules. The normalised spectral gradient of reflectivity is 2.8% per 1000 Å and 5.4% per 1000 Å for November 14 and 21, respectively. The Afρ parameter, which characterises the dust production rate in the comet, is on average about 800 cm. Comet C/2002 T7 (LINEAR) can be classified as belonging to the group of dusty comets
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Advances in Astronomy and Space Physics
Advances in Astronomy and Space Physics ASTRONOMY & ASTROPHYSICS-
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