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Binary star system in the constellation Scutum
LS 5039 is a binary system in the constellation of Scutum. It has an apparent magnitude of 11.27, and it is about 8,200 light-years away. The "LS" in
LS_5039
Upper bound to the mass of cold, nonrotating neutron stars
J; Herrero, A (2005). "A possible black hole in the γ-ray microquasar LS 5039". Monthly Notices of the Royal Astronomical Society. 364 (3): 899–908.
Tolman–Oppenheimer–Volkoff limit
Tolman–Oppenheimer–Volkoff_limit
Star in the constellation Cassiopeia
that produce such energetic rays. Other such systems are PSR B1259–63, LS 5039 and HESS J0632+057. Roman, Nancy G. (1987). "Identification of a constellation
LS_I_+61_303
X-3 (V1521) CI Cam GRS 1915+105 GRO J1655-40 GX339-4 KS1731-260 LS I +61 303 LS 5039 Scorpius X-1 SS 433 V404 Cygni V4641 Sgr V691 CrA XMMU J004243.6+412519
List_of_microquasars
5.34 - 5.45 Has a A-type Hypergiant Companion. HD 93160 8,000 1 O6III LS 5039 A 8200±300 1 O(f)N6.5V 11.27 Has a Black Hole Companion. WR 22 B 8,300
List_of_O-type_stars
V476 18h 32m 04.75s −06° 43′ 34.3″ 11.10 nova, Vmax = 11.1m, Vmin = <17m LS 5039 V479 18h 26m 15.06s −14° 50′ 54.3″ 11.23 O(f)N6.5V High-mass X-ray binary;
List_of_stars_in_Scutum
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