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|
HD 326823, also known as V1104 Scorpii, is … HD 326823, also known as V1104 Scorpii, is a binary star containing a unique emission-line star, which is in the midst of transitioning to a nitrogen-rich Wolf-Rayet star, as well as being a candidate Luminous blue variable, located 4,142 light years away in the constellation of Scorpius. The primary is very evolved, because it is composed of almost entirely helium, and only 3% of it is still hydrogen, and it has lost most of its mass to the now-very-massive secondary. The underlying mechanisms and mass transfers in the system are comparable to other W Serpentis systems, such as Beta Lyrae and .erpentis systems, such as Beta Lyrae and .
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69522708
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7173
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WN
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http://dbpedia.org/resource/Scorpius +
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1270
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0.17
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J2000.0
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45
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80000
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29.1
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0.0193
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0.6919
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529009.9199999999
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−2.251
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+2.545
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10
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22000
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| rdfs:comment |
HD 326823, also known as V1104 Scorpii, is … HD 326823, also known as V1104 Scorpii, is a binary star containing a unique emission-line star, which is in the midst of transitioning to a nitrogen-rich Wolf-Rayet star, as well as being a candidate Luminous blue variable, located 4,142 light years away in the constellation of Scorpius. The primary is very evolved, because it is composed of almost entirely helium, and only 3% of it is still hydrogen, and it has lost most of its mass to the now-very-massive secondary. The underlying mechanisms and mass transfers in the system are comparable to other W Serpentis systems, such as Beta Lyrae and .erpentis systems, such as Beta Lyrae and .
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| rdfs:label |
HD 326823
|
