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AS 314
Protoplanetary nebula in the constellation Scutum From Wikipedia, the free encyclopedia
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AS 314, also known as V452 Scuti, is a protoplanetary nebula[4] once believed to be a white hypergiant star or luminous blue variable located in the constellation of Scutum. It has an apparent magnitude of 9.85 and can be seen with small telescopes.
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Characteristics
AS 314 was found to be a variable star in 1996, when the Hipparcos data was analyzed. For that reason it was given the variable star designation V452 Scuti, in 1999.[7]
AS 314 was poorly studied until the year 2000, when Miroshnichenko et al. incorrectly estimated a distance for this star of around 10 kiloparsecs (32,600 light years), a luminosity 160,000 times that of Sun (L☉), a radius 200 times the solar radius (R☉), and an initial mass of 20 solar masses (M☉). It was also estimated to be losing 2 × 10−5 M☉ each year (in other words, 1 M☉ every 50,000 years) through a very strong stellar wind.[8]
AS 314 has an infrared excess, suggesting that it is shrouded in a circumstellar envelope of dust.[8][9] However, it has not been classified as a bona fide luminous blue variable, but as a candidate.[10]
The Hipparcos parallax and proper motions are large and imply a much closer, and hence less luminous, star.[11] The Hipparcos measurement was later confirmed by the Gaia mission,[2] reclassifying AS 314 as post-AGB star.[4]
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References
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