Emission nebula | |
---|---|
Planetary nebula | |
Observation data: J2000 epoch | |
Right ascension | 15h 37m 11.2s [1] |
Declination | −71° 54′ 52.9″ [1] |
Distance | 2200 [2] pc |
Apparent magnitude (V) | 10.47 [1] |
Constellation | Apus |
Physical characteristics | |
Absolute magnitude (V) | - |
Notable features | - |
Hen 2-131 is a planetary nebula in the southern constellation of Apus. It was discovered by Andrew David Thackeray in 1950 [3] and added to the Catalogues of Hα-emission Stars and Nebulae in the Magellanic Clouds by Karl Gordon Henize in 1967. [4]
Hen 2-131 is about 2,200 pc from earth. [2] HD 138403 is the star located in the center of Hen 2–131 with a spectral type of O8(f)ep. [5] The nebula expands at a speed of 11.5 km/s, and the temperature of HD 138403 is about 34,000 K. HD 138403 is suspected of variability, possibly by 0.1 to 0.15 magnitudes over a period of several hours. This nebula is similar to IC 418, IC 4593 and Hen 2-138. [6]
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Emission nebula | |
---|---|
Planetary nebula | |
Observation data: J2000 epoch | |
Right ascension | 15h 37m 11.2s [1] |
Declination | −71° 54′ 52.9″ [1] |
Distance | 2200 [2] pc |
Apparent magnitude (V) | 10.47 [1] |
Constellation | Apus |
Physical characteristics | |
Absolute magnitude (V) | - |
Notable features | - |
Hen 2-131 is a planetary nebula in the southern constellation of Apus. It was discovered by Andrew David Thackeray in 1950 [3] and added to the Catalogues of Hα-emission Stars and Nebulae in the Magellanic Clouds by Karl Gordon Henize in 1967. [4]
Hen 2-131 is about 2,200 pc from earth. [2] HD 138403 is the star located in the center of Hen 2–131 with a spectral type of O8(f)ep. [5] The nebula expands at a speed of 11.5 km/s, and the temperature of HD 138403 is about 34,000 K. HD 138403 is suspected of variability, possibly by 0.1 to 0.15 magnitudes over a period of several hours. This nebula is similar to IC 418, IC 4593 and Hen 2-138. [6]
{{
cite book}}
: |journal=
ignored (
help)