Frosty Leo Nebula
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Protoplanetary nebula | Lists of nebulae |
---|---|
Observation data (Epoch J2000) |
|
Right ascension | 09h 39m 53.96s[1] |
Declination | +11° 58′ 52.4″[1] |
Distance | 3 kly (920 pc)[2] |
Apparent magnitude (V) | |
Apparent dimensions (V) | |
Constellation | Leo |
Physical characteristics | |
Radius | ? ly[a] |
Absolute magnitude (V) | ?[b] |
Notable features | - |
Other designations | IRAS 09371+1212[1] |
The Frosty Leo Nebula is a protoplanetary nebula located roughly at 3,000 light-years (Davis et al. 2005) away from Earth. It is a bipolar nebula. Its central star is of spectral type K7II. It is unusual in that it has an extremely deep absorption feature at 3.1µm and is unusually located at more than 900 pc above the plane of our galaxy.(Bourke et al. 2000)
[edit] Notes
- ^ distance × sin( diameter_angle / 2 ) = ? ly. radius
- ^ ?[1] apparent magnitude - 5 * (log10(920 pc distance) - 1) = ? absolute magnitude
- ^ a b c d (SIMBAD 2007)
- ^ (Davis et al. 2005)
[edit] References
- Davis, C. J.; M. D. Smith & T. M. Gledhill et al. (2005), "Near-infrared echelle spectroscopy of protoplanetary nebulae: probing the fast wind in H2", Monthly Notices of the Royal Astronomical Society 360(1): 104-118
- Bourke, Tyler; A. R. Hyland & Garry Robinson et al. (2000), "The Evolutionary Status of the Frosty Leo Nebula", Asymmetrical Planetary Nebulae II: From Origins to Microstructures, ASP Conference Series. Edited by J. H. Kastner, N. Soker, and S. Rappaport. ISBN: 1-58381-026-9 199(1): 171
- SIMBAD (January 7, 2007), Results for Frosty Leo Nebula, SIMBAD, Centre de Données Astronomiques de Strasbourg