A REMARKABLE FEATURE IN THE GIANT EXTRAGALACTIC H-II REGION NGC 5471

被引:40
作者
CASTANEDA, HO
VILCHEZ, JM
COPETTI, MVF
机构
[1] ROYAL GREENWICH OBSERV,CAMBRIDGE CB3 0EZ,ENGLAND
[2] UNIV FED SANTA MARIA,DEPT MATEMAT NEPAE,SANTA MARIA,RS,BRAZIL
关键词
Galaxies: individual (NGC 5471); Galaxies: interstellar matter; Nebulae: H II regions; Nebulae: internal motions;
D O I
10.1086/169466
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of a very high velocity, low-intensity gas feature in the giant extragalactic H II region NGC 5471. A broad component in the emission lines of Hα + [N II] λλ6548, 6584 is located within an area less than 1″ in diameter at the position known as knot C. The broad component is characterized by its low intensity (less than 2% of the peak surface brightness in Hα), a contribution of ≈25% to the total flux of the lines, and an extension of ≈3300 km s-1 at full width at zero intensity (FWZI). Supernovae explosions and stellar winds are considered as possible sources of the gas motions, and the observational evidence for their presence is discussed.
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页码:164 / 167
页数:4
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