A H13CN/HN13C linelist, model atmospheres and synthetic spectra for carbon stars

被引：52

作者：

Harris, G. J. ^{[1
]}

Larner, F. C. ^{[1
]}

Tennyson, J. ^{[1
]}

Kaminsky, B. M. ^{[2
]}

Pavlenko, Ya. V. ^{[2
]}

Jones, H. R. A. ^{[3
]}

机构：

[1] UCL, Dept Phys & Astron, London WC1E 6BT, England

[2] Natl Acad Sci, Main Astron Observ, UA-03680 Kiev 127, Ukraine

[3] Univ Hertfordshire, Ctr Astrophys Res, Hatfield AL10 9AB, Herts, England

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2008年 / 390卷 / 01期

关键词：

molecular data; stars: AGB and post-AGB; stars: atmospheres; stars: carbon; infrared: stars;

D O I：

10.1111/j.1365-2966.2008.13642.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A linelist of vibration-rotation transitions for C-13 substituted HCN is presented. The linelist is constructed using known experimental levels where available, calculated levels and ab initio line intensities originally calculated for the major isotopologue. Synthetic spectra are generated and compared with observations for cool carbon star WZ Cas. It is suggested that high resolution HCN spectra recorded near 14 mu m should be particularly sensitive to the C-13-C-12 ratio.

引用

页码：143 / 148

页数：6

共 50 条

[1] H13CN–HN13C Intensity Ratio as a Temperature Indicator of Interstellar Clouds
A. G. Pazukhin
I. I. Zinchenko
E. A. Trofimova
C. Henkel
Astronomy Reports, 2022, 66 : 1302 - 1310
[2] MODEL ATMOSPHERES SYNTHETIC SPECTRA - H-C-N-O ABUNDANCE RATIO IN CARBON STARS
QUERCI, M
QUERCI, F
ASTRONOMY & ASTROPHYSICS, 1976, 49 (03) : 443 - 462
[3] Synthetic Spectra for Carbon Stars from Dynamica Model Atmospheres
Rita Loidl
Josef Hron
Bernhard Aringer
Susanne Höfner
Uffe G. Jφrgensen
Astrophysics and Space Science, 1997, 255 (1-2) : 289 - 290
[4] Synthetic spectra for carbon stars from dynamical model atmospheres
Loidl, R
Hron, J
Aringer, B
Hofner, S
Jorgensen, UG
ASTROPHYSICS AND SPACE SCIENCE, 1998, 255 (1-2) : 289 - 290
[5] H13CN-HN13C Intensity Ratio as a Temperature Indicator of Interstellar Clouds
Pazukhin, A. G.
Zinchenko, I. I.
Trofimova, E. A.
Henkel, C.
ASTRONOMY REPORTS, 2022, 66 (12) : 1302 - 1310
[6] DETECTIONS OF C2H, CYCLIC-C3H2, AND H13CN IN NGC 1068
Nakajima, T.
Takano, S.
Kohno, K.
Inoue, H.
ASTROPHYSICAL JOURNAL LETTERS, 2011, 728 (02)
[7] Dynamic model atmospheres of AGB stars -: II.: Synthetic near infrared spectra of carbon stars
Loidl, R
Höfner, S
Jorgensen, UG
Aringer, B
ASTRONOMY & ASTROPHYSICS, 1999, 342 (02) : 531 - 541
[8] ALMA Autocorrelation Spectroscopy of Comets: The HCN/H13CN Ratio in C/2012 S1 (ISON)
Cordiner, M. A.
Palmer, M. Y.
de Val-Borro, M.
Charnley, S. B.
Paganini, L.
Villanueva, G.
Bockelee-Morvan, D.
Biver, N.
Remijan, A. J.
Kuan, Y. -J.
Milam, S. N.
Crovisier, J.
Lis, D. C.
Mumma, M. J.
ASTROPHYSICAL JOURNAL LETTERS, 2019, 870 (02)
[9] Dynamic model atmospheres of AGB stars IV. A comparison of synthetic carbon star spectra with observations
Gautschy-Loidl, R. (rita@gautschy.ch), 1600, EDP Sciences (422):
[10] Dynamic model atmospheres of AGB stars -: IV.: A comparison of synthetic carbon star spectra with observations
Gautschy-Loidl, R
Höfner, S
Jorgensen, UG
Hron, J
ASTRONOMY & ASTROPHYSICS, 2004, 422 (01): : 289 - 306

← 1 2 3 4 5 →