NEUTRAL CARBON FAR-RED FORBIDDEN LINE EMISSION FROM PLANETARY-NEBULAE

被引:21
作者
LIU, XW
BARLOW, MJ
DANZIGER, IJ
CLEGG, RES
机构
[1] EUROPEAN SO OBSERV,D-85748 GARCHING,GERMANY
[2] ROYAL GREENWICH OBSERV,CAMBRIDGE CB3 0EZ,ENGLAND
关键词
LINE FORMATION; PLANETARY NEBULAE; GENERAL;
D O I
10.1093/mnras/273.1.47
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The temperature-sensitive neutral carbon forbidden lines at 8727, 9824 and 9850 Angstrom have been measured simultaneously for the first time from a planetary nebula. The nebulae NGC 2346, NGC 2440, NGC 3132 and IC 4406 were observed. Accurate rest wavelengths of these lines are obtained. The observed line ratios I[lambda 9824 + lambda 9850]/I[lambda 8727] are consistent with collisional excitation by electron impacts. It is demonstrated that radiative recombination and stellar continuum fluorescence are unimportant in exciting the observed [C I] lines, with the possible exception of NGC 2440 where a contribution from the former process cannot be ruled out. For NGC 2346, NGC 3132 and IC 4406, the observed [C I] line ratios yield electron temperatures between 7400 and 8000 K, about 1800 to 2800 K lower than those deduced from the [N II], [S III] and [O III] Line ratios that we also measured. Electron densities are derived from the observed [N I], [S II] and [Cl III] doublet ratios.
引用
收藏
页码:47 / 58
页数:12
相关论文
共 42 条
  • [31] Mapping low- and high-density clouds in astrophysical nebulae by imaging forbidden line emission
    Steiner, J. E.
    Menezes, R. B.
    Ricci, T. V.
    Oliveira, A. S.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2009, 396 (02) : 788 - 793
  • [32] New detected CO (1-0) emission from planetary nebulae
    孙锦
    孙艳春
    Science China Mathematics, 2000, (02) : 217 - 224
  • [33] New detected CO(1-0) emission from planetary nebulae
    Jin Sun
    Yanchun Sun
    Science in China Series A: Mathematics, 2000, 43 : 217 - 224
  • [34] New detected CO(1-0) emission from planetary nebulae
    Sun, J
    Sun, YC
    SCIENCE IN CHINA SERIES A-MATHEMATICS PHYSICS ASTRONOMY, 2000, 43 (02): : 217 - 224
  • [35] Simulations of the Formation and X-ray Emission from Hot Bubbles in Planetary Nebulae
    Toala, Jesus A.
    Jane Arthur, S.
    GALAXIES, 2018, 6 (03):
  • [36] Carbon-rich dust from the asymptotic giant branch to planetary nebulae
    Sloan, G. C.
    PLANETARY AND SPACE SCIENCE, 2017, 149 : 32 - 37
  • [37] DETECTION OF THE H92-ALPHA RECOMBINATION LINE TOWARD THE VERY COMPACT PLANETARY-NEBULAE IC-5117 AND HB-12
    MIRANDA, LF
    TORRELLES, JM
    EIROA, C
    ASTROPHYSICAL JOURNAL, 1995, 446 (01) : L39 - L42
  • [38] A Survey of 3-5.4μm Emission from Planetary Nebulae Using SOFIA/FLITECAM
    Smith, Erin C.
    Logsdon, Sarah E.
    McLean, Ian S.
    Fletcher, Elizabeth
    Vacca, William D.
    Becklin, E. E.
    Shenoy, Sachindev
    Savage, Maureen
    Hamilton, Ryan T.
    ASTROPHYSICAL JOURNAL, 2020, 902 (02)
  • [39] CARBON-MONOXIDE EMISSION FROM THE PLANETARY-NEBULA M3-28
    GOMEZ, Y
    RODRIGUEZ, LF
    GARAY, G
    ASTRONOMY & ASTROPHYSICS, 1992, 258 (02) : 469 - 471
  • [40] Evolution of carbon particles from the stage of asymptotic giant branch stars to planetary nebulae: observations, experiments, and theory
    Murga, M. S.
    PHYSICS-USPEKHI, 2024, 67 (10) : 961 - 987