Circinus X-1
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| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Circinus |
| Right ascension | Template:RA[1] |
| Declination | Template:DEC[1] |
| Apparent magnitude (V) | 21.40[2] |
| Characteristics | |
| Spectral type | B5–A0 I[3] |
| Variable type | HMXB[4] |
| Astrometry | |
| Distance | Script error: No such module "val". ly (Script error: No such module "val".[5] pc) |
| Orbit[3] | |
| Period (P) | 16.68 ± 0.15 d |
| Eccentricity (e) | 0.45 ± 0.07 |
| Periastron epoch (T) | JD 2453473.8 ± 0.4 |
| Argument of periastron (ω) (secondary) | 2 ± 12° |
| Semi-amplitude (K1) (primary) | 25 ± 2 km/s |
| Other designations | |
| Template:Odlist[4] | |
| Database references | |
| SIMBAD | data |
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Circinus X-1 is an X-ray binary star system that includes a neutron star. Observation of Circinus X-1 in July 2007 revealed the presence of X-ray jets normally found in black hole systems; it is the first of the sort to be discovered that displays this similarity to black holes. Circinus X-1 may be among the youngest X-ray binaries observed.
Location, distance
On June 14, 1969, an Aerobee 150 rocket, launched from Natal, Rio Grande do Norte, Brazil, obtained X-ray data during a scan of the Norma-Lupus-Circinus region that detected a well-isolated source at ℓ = 321.4±0.9° b = -0.5±2° (galactic), RA Template:RA Dec Script error: No such module "String".° 49′ within the constellation Circinus and referred to as Circinus XR-1 (Cir XR-1).[6] The distance of Circinus X-1 was not well established, with a low estimate of 13,400 light years[7] and high estimate of 26,000 light years.[8]
On June 23, 2015, an article published on NASA's Chandra X-Ray Observatory's website, revealed that an international team of astronomers has succeeded in determining its distance from Earth with more precision - via a method of triangulation of X-ray light emitted by the star, echoing through stellar clouds and interstellar dust - as being about 30,700 light-years.[9]
A 16.6 day X-ray period was found by Kaluzienski et al.[11] The X-ray source is assumed to be a neutron star as part of a low-mass X-ray binary (LMXB), type-I X-ray burster.[12] The X-ray and radio nebulae surrounding Circinus X-1 have properties consistent with a young supernova remnant. This rare case of an X-ray binary apparently associated with a supernova remnant suggests the binary is very young on cosmic time scales, possibly less than 4600 years old.[13] An association of Circinus X-1 with a different nearby supernova remnant, G321.9-0.3, has been ruled out.[12]
Other spectral regions
The binary nature of Cir X-1 has been established.[14] The binary's radio component and a possible visual counterpart were identified by Whelan et al.[15] Its infrared counterpart was located and found to flare with a 16.6-day period by Glass.[16] A (heavily reddened) precise optical counterpart (now known as BR Cir) was identified by Moneti.[17]
References
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External links
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