On the CH B-X (1, 0) band in translucent clouds

T.; Weselak; G. Galazutdinov; Y. Beletsky; J. Krełowski

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On the CH B-X (1, 0) band in translucent clouds

机译：在半透明云的CH B-X（1，0）波段上

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We present observations of CH B-X (1, 0) band toward 13 translucent sightlines. The given precise positions (at 3627.403, 3633.289, 3636.222 Å) are derived by means of shifting our spectra to the rest velocity frame using B-X (0, 0) features (at 3878, 3886 and 3890 Å). The proposed oscillator strengths (equal to 0.00035, 0.00104, 0.00069, respectively) are based on f -values of the CH B-X (0, 0) system, i.e. 0.00110, 0.00320, 0.00210 (© 2011 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)

机译：我们向13个半透明视线展示了CH B-X（1，0）波段的观测结果。通过使用B-X（0，0）功能（在3878、3886和3890Å）将光谱移至静止速度帧，可以得出给定的精确位置（在3627.403、3633.3289、3636.22Å处）。建议的振荡器强度（分别等于0.00035、0.00104和0.00069）基于CH BX（0，0）系统的f值，即0.00110、0.00320、0.00210（©2011 WILEY-VCH Verlag GmbH＆Co. KGaA ，魏因海姆（Weinheim）

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来源
《Astronomische Nachrichten》 |2011年第2期|p.167-171|共5页
作者
T.; Weselak; G. Galazutdinov; Y. Beletsky; J. Krełowski;
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作者单位

Institute of Physics, Kazimierz Wielki University, Weyssenhoffa 11, 85-072 Bydgoszcz, Poland;

Institute of Physics, Kazimierz Wielki University, Weyssenhoffa 11, 85-072 Bydgoszcz, Poland;

Instituto de Astronomia, Universidad Catolica del Norte, Angamos 0610, Antofagasta, Chile;

European Southern Observatory (ESO), Alonso de Cordova 3107, Santiago, Chile;

Center for Astronomy, Nicolaus Copernicus University, Gagarina 11, Pl-87-100 Toruń, Poland;

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正文语种 eng
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关键词
ISM: clouds; ISM: lines and bands; ISM: molecules;

机译：ISM：云;ISM：线和带;ISM：分子;

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专利

1. On the CH B-X (1, 0) band in translucent clouds [J] . T. Weselak, G. Galazutdinov, Y. Beletsky, Astronomische Nachrichten: A Journal on all Fields of Astronomy . 2011,第2期

机译：在半透明云的CH B-X（1，0）波段上
2. MECHANISMS FOR THE ORIGIN OF TURBULENCE IN NON-STAR-FORMING CLOUDS: THE TRANSLUCENT CLOUD MBM 40 [J] . STEVEN N. SHORE, LORIS MAGNANI, T. N. LAROSA, The Astrophysical journal . 2003,第1aaParta1期

机译：非星形云中湍流起源的机制：半透明云MBM 40
3. Mechanisms for the Origin of Turbulence in Non-Star-forming Clouds: The Translucent Cloud MBM 40 [J] . Steven N. Shore, Loris Magnani, T. N. LaRosa, The Astrophysical journal . 2003,第1期

机译：非恒星形成云中湍流起源的机制：半透明云MBM 40
4. Simultaneous PLIF and Cavity Ringdown Absorption Measurements of CN(B-X) and CH(B-X) in Low Pressure CH_4-O_2-N_2 and CH_4-NO-O_2-N_2 Flames. [C] . J. Luque, J.B. Jeffries, G.P. Smith, Spring 2000 meeting of the Western States Section of the Combustion Institute (WSS/CI spring 2000) . 2000

机译：CN（B-X）和CH（B-X）在低压CH_4-O_2-N_2和CH_4-NO-O_2-N_2火焰中同时PLIF和腔衰荡吸收测量。
5. Comparison of convective clouds observed by spaceborne W-band radar and simulated by cloud-resolving atmospheric models. [D] . Dodson, Jason B. 2014

机译：机载W波段雷达观测到的对流云比较，并通过云解析大气模型进行了模拟。
6. Organic Molecules in Translucent Interstellar Clouds [O] . Jacek Krełowski -1

机译：半透明星际云中的有机分子
7. Detection of vibronic bands of C$_3$ in a translucent cloud towards HD 169454 [O] . Schmidt, M. R., Krełowski, J., Galazutdinov, G. A., 2014

机译：在半透明的云中向HD检测C $ _3 $的电子乐队频段 169454
8. Laser Excitation of the Overlapping CN B-A (8, 7) and B-X (8, 11) Bands: The Relative Phase of the B-A and B-X Transition Moments [R] . Furio, N., Ali, A., Dagdigian, P. J., 1989

机译：重叠CN B-a（8,7）和B-X（8,11）带的激光激发：B-a和B-X跃迁矩的相对相位

On the CH B-X (1, 0) band in translucent clouds

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