Midcourse Space Experiment Spectra of the Orion Nebula and the Implications for Abundances in the Interstellar Medium
暂无分享,去创建一个
S. Price | F. Witteborn | J. Simpson | M. Cohen | Stephan D. Price | Marvin L. Cohen | Janet P. Simpson
[1] C. Esteban,et al. Chemical composition of the Orion nebula derived from echelle spectrophotometry , 1998 .
[2] Martin G. Cohen,et al. A Population of Cold Cores in the Galactic Plane , 1998 .
[3] K. Widing. Emerging Active Regions on the Sun and the Photospheric Abundance of Neon , 1997 .
[4] J. Mathis. Dust Models with Tight Abundance Constraints , 1996 .
[5] H. Kataza,et al. Fabry-Perot Imaging of H 2 1--0 S(1), 2--1 S(1), and Brackett-Gamma Emission in the Orion Nebula , 1996 .
[6] M. R. Haas,et al. Far-infrared lines from H II regions: Abundance variations in the galaxy , 1995 .
[7] D. Hudgins,et al. Infrared spectroscopy of matrix-isolated polycyclic aromatic hydrocarbon cations. 2. The members of the thermodynamically most favorable series through coronene. , 1995, The Journal of physical chemistry.
[8] J. Miles,et al. Thermal infrared imaging of subarcsecond structure in the trapezium nebula , 1994 .
[9] O. Manuel Uy,et al. Midcourse Space Experiment: Introduction to the Spacecraft, Instruments, and Scientific Objectives , 1994 .
[10] J. Lacy,et al. Shocked pure-rotational emission from H2 in Orion , 1994 .
[11] K. Cunha,et al. Chemical evolution of the Orion association. II. The carbon, nitrogen, oxygen, silicon, and iron abundances of main-sequence B stars , 1994 .
[12] R. Rubin,et al. Silicon and carbon abundances in the Orion nebula , 1993 .
[13] S. Veilleux,et al. Faint emission lines in the spectrum of the Orion Nebula and the abundances of some of the rarer elements , 1992 .
[14] T. Wilson,et al. Abundances in the interstellar medium , 1992 .
[15] D. Smits. Theoretical He I line intensities in low-density plasmas , 1991 .
[16] M. R. Haas,et al. Axisymmetric model of the ionized gas in the Orion Nebula , 1991 .
[17] J. Baldwin,et al. Physical conditions in the Orion Nebula and an assessment of its helium abundance , 1991 .
[18] J. Lacy,et al. Detection of low-J pure-rotational emission from H2 in the Orion Bar region - Evidence for small-scale clumpiness , 1991 .
[19] R. Rubin,et al. IRAS Low-Resolution Spectral Observations of H II Regions , 1990 .
[20] A. Tielens,et al. Interstellar polycyclic aromatic hydrocarbons: the infrared emission bands, the excitation/emission mechanism, and the astrophysical implications. , 1989, The Astrophysical journal. Supplement series.
[21] A. Tielens,et al. The infrared emission bands. II. A spatial and spectral study of the Orion Bar. , 1989, The Astrophysical journal.
[22] L. Allamandola,et al. The infrared emission bands. III. Southern IRAS sources. , 1989, The Astrophysical journal.
[23] S. Sandford,et al. New emission features in the 11-13 micron region and their relationship to polycyclic aromatic hydrocarbons. , 1989, The Astrophysical journal.
[24] J. Stutzki,et al. The Orion Molecular Cloud and Star-Forming Region , 1988 .
[25] A. Tielens,et al. Anharmonicity and the interstellar polycyclic aromatic hydrocarbon infrared emission spectrum , 1987 .
[26] C. Johnson,et al. Atomic data for the S IV 10.5-μm fine-structure transition , 1986 .
[27] A. Tielens,et al. The infrared emission bands. I - Correlation studies and the dependence on C/O ratio. [in planetary and reflection nebulae and H II regions] , 1986 .
[28] H. M. Lee,et al. Optical properties of interstellar graphite and silicate grains , 1984 .
[29] P. Roche,et al. 8–13 μm spectrophotometry of compact planetary nebulae and emission line objects , 1982 .
[30] David A. Williams,et al. The infrared spectrum of interstellar dust: Surface functional groups on carbon , 1981 .
[31] M. Peimbert,et al. Chemical composition of the Orion Nebula. , 1977 .
[32] D. G. Hummer,et al. Recombination line intensities for hydrogenic ions-IV. Total recombination coefficients and machine-readable tables for Z=1 to 8 , 1995 .
[33] D. Hudgins,et al. Infrared spectroscopy of matrix-isolated polycyclic aromatic hydrocarbon cations. 3. The polyacenes anthracene, tetracene, and pentacene. , 2013, The Journal of physical chemistry.
[34] D. Osterbrock,et al. Astrophysics of Gaseous Nebulae and Active Galactic Nuclei , 1989 .
[35] A. Dalgarno,et al. The Quadrupole Vibration-Rotation Transition Probabilities of Molecular Hydrogen , 1977 .