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GCIRS 16SW

GCIRS 16SW, also known as S97, is a contact binary star located in the Galactic Center. It is composed of two hot massive stars of equal size that orbit

GCIRS 13E

(IMBH) at its center. GCIRS 13E was first identified as GCIRS 13, which was later resolved into two components GCIRS13E and W. GCIRS 13E was initially modelled

GCIRS 7

GCIRS 7 is a pulsating red supergiant star located in the Galactic Center of the Milky Way galaxy. It is very luminous with a luminosity of 189,000 Sun's

Sagittarius A*

the discovery of a potential intermediate-mass black hole, referred to as GCIRS 13E, orbiting 3 light-years from Sagittarius A*. This black hole of 1,300

GCIRS 8*

GCIRS 8* (Galactic Centre IRS 8*) is a young massive star in the Galactic Center region. IRS 8 is an infra-red source identified as a bowshock. The star

Planets in astrology

home to colossal red supergiants such as KW Sagittarii, VX Sagittarii, and GCIRS 7, all of which are roughly the size of Jupiter's orbit. In astrology, Jupiter

Sagittarius A* cluster

1.60 1108.000 69.000 958.0 50.0 12.20 10928.4 74.5 0.22 0.02 S96 S0-96 GCIRS 16C Ofpe/WN9 1.4990 0.0570 0.1740 0.0220 126.36 0.96 115.66 0.59 233.60

HD 163296

Listen Pulsar Bursting Pulsar CEN 16 CWISEP J1935−1546 D9 GCIRS 7 GCIRS 8* GCIRS 13E GCIRS 16SW Gomez's Hamburger G0.238−0.071 HATS-36 IRAS 17423−1755

List of most luminous stars

Sellgren, K. (2007-01-01). "The Nature of the Variable Galactic Center Source GCIRS 16SW Revisited: A Massive Eclipsing Binary". The Astrophysical Journal.