期刊
ASTRONOMY & ASTROPHYSICS
卷 415, 期 2, 页码 L27-L30出版社
E D P SCIENCES
DOI: 10.1051/0004-6361:20040006
关键词
galaxies : abundances; galaxies : dwarf; galaxies : evolution; galaxies : compact; galaxies : starburst; galaxies : stellar content; galaxies : individual Tol 1214-277
The discovery of the high-ionization [Ne V] lambda3426 Angstrom emission line in the spectrum of the blue compact dwarf (BCD) galaxy Tol 1214-277 is reported. The detection of this line implies the presence of intense ionizing X-ray emission with a luminosity L-x in the range 10(39)-10(40) erg s(-1), Such a high X-ray luminosity cannot be reproduced by models of massive stellar populations. Other mechanisms, such as fast shocks or accretion of gas in high-mass X-ray binaries need to be invoked to account for the high intensity of the [Ne V] lambda3426 Angstrom emission line.
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