1806−20 cluster
1806−20 (originally named the SGR 1806−20 cluster) is a heavily obscured star cluster on the far side of the Milky Way, approximately 50,000 light-years distant. It contains the soft gamma repeater SGR 1806−20 and the luminous blue variable hypergiant LBV 1806−20, a candidate for the most luminous star in the Milky Way. LBV 1806−20 and many of the other massive stars in the cluster are thought likely to end as supernovas in a few million years, leaving only neutron stars or black holes as remnants.
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1806−20 cluster
1806−20 (originally named the SGR 1806−20 cluster) is a heavily obscured star cluster on the far side of the Milky Way, approximately 50,000 light-years distant. It contains the soft gamma repeater SGR 1806−20 and the luminous blue variable hypergiant LBV 1806−20, a candidate for the most luminous star in the Milky Way. LBV 1806−20 and many of the other massive stars in the cluster are thought likely to end as supernovas in a few million years, leaving only neutron stars or black holes as remnants.
has abstract
1806-20 est un amas ouvert sit ...... 20 et le magnétar SGR 1806-20.
@fr
1806-20（最初命名為SGR 1806-20星團）是在銀 ...... WN6、和WN7）和OB型超巨星，加上其它年輕的大質量恆星。
@zh
1806−20 (originally named the ...... lus other young massive stars.
@en
Cl* 1806-20 é um aglomerado es ...... es de estrelas jovens massivas
@pt
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17,914,618
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1,022,270,567
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constellation
Sagittarius
@en
dist ly
~50000 ly
@en
dist pc
~15000 pc
@en
epoch
J2000
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names
G10.0-0.3, W31
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notes
Contains SGR 1806−20 and LBV 1806−20.
@en
wikiPageUsesTemplate
comment
1806-20 est un amas ouvert sit ...... 20 et le magnétar SGR 1806-20.
@fr
1806-20（最初命名為SGR 1806-20星團）是在銀 ...... WN6、和WN7）和OB型超巨星，加上其它年輕的大質量恆星。
@zh
1806−20 (originally named the ...... rs or black holes as remnants.
@en
Cl* 1806-20 é um aglomerado es ...... cos negros como remanescentes.
@pt
label
1806-20
@fr
1806-20星團
@zh
1806−20 cluster
@en
Cl* 1806-20
@pt
성단 1806-20
@ko