Abstract
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.
Original language | English |
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Pages (from-to) | 164-167 |
Number of pages | 4 |
Journal | Astrophysical Journal |
Volume | 365 |
Issue number | 1 |
DOIs | |
State | Published - 10 Dec 1990 |
Externally published | Yes |
Keywords
- Galaxies: individual (NGC 5471)
- Galaxies: interstellar matter
- Nebulae: H II regions
- Nebulae: internal motions