RX J1856.5−3754
File:RX J1856.5-3754.jpg X-ray image of RX J1856.5−3754 | |
| Observation data Epoch 1996.7 Equinox J2000.0[1] | |
|---|---|
| Constellation | Corona Australis |
| Right ascension | Template:RA[1] |
| Declination | Template:DEC[1] |
| Apparent magnitude (V) | ~25.6[1] |
| Details | |
| Mass | [2] Template:Solar mass |
| Radius | [2] km |
| Age | 1 Myr |
| Metallicity [Fe/H] | {{{metal_fe2}}} dex |
| Other designations | |
| RX J185635−3754, 1ES 1853−37.9, 1RXS J185635.1−375433 | |
| Database references | |
| SIMBAD | data |
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RX J1856.5−3754 (also called RX J185635−3754, RX J185635−375, and various other designations) is a neutron star in the constellation Corona Australis. At approximately 400 light-years from Earth, it is the closest neutron star discovered to date.
Discovery and location
RX J1856.5−3754 is thought to have formed in a supernova explosion of its companion star about one million years ago and is moving across the sky at Script error: No such module "val".. It was discovered in 1992, and observations in 1996 confirmed that it is a neutron star, the closest to Earth discovered to date.[3]
It was originally thought to be about 150–200 light-years away,[4] but further observations using the Chandra X-ray Observatory in 2002 indicate that its distance is greater—about 400 light-years.[5][6]
RX J1856 is one of the Magnificent Seven, a group of young neutron stars at distances between Script error: No such module "convert". of Earth.
Quark star hypothesis
By combining Chandra X-ray Observatory and Hubble Space Telescope data, astronomers previously estimated that RX J1856 radiates like a solid body with a temperature of Script error: No such module "val". and has a diameter of about Script error: No such module "val".. This estimated size was too small to reconcile with the standard models of neutron stars, and it was therefore suggested that it might be a quark star.[5]
However, later refined analysis[6][7] of improved Chandra and Hubble observations revealed that the surface temperature of the star is lower, only Script error: No such module "val"., and, consequently, the radius is larger, about Script error: No such module "val". (the observed radius appears about Script error: No such module "val". due to general-relativistic effects).[6] Thus, RX J1856.5–3754 is now excluded from the list of quark star candidates.[7] A subsequent more accurate parallax estimation has led to the correction of this result to Script error: No such module "val". for the true radius (and about Script error: No such module "val". for the observed radius).[2]
Vacuum birefringence
In 2016 a team of astronomers from Italy, Poland, and the UK using the Very Large Telescope reported[9][10] observational indications of vacuum birefringence from RX J1856.5−3754. A degree of polarization of about 16% was measured from the visible spectrum being large enough to support evidence but not discovery due to the low accuracy of star model and the uncertain direction of the neutron magnetization axis.[11]
Its inferred magnetic field of Script error: No such module "val". should produce a greater effect at X-ray wavelengths, which could be measured by future planned polarimeters, such as NASA's Imaging X-ray Polarimeter Explorer (IXPE), NASA's Polarimetry of Relativistic X-ray Sources (PRAXYS), or ESA's X-ray Imaging Polarimetry Explorer (XIPE).[12]
See also
- 3C 58, a possible quark star
References
- RX-J185635-375 at jumk.de
- RX J1856.5-3754 and 3C58: Cosmic X-rays May Reveal New Form of Matter Chandra X-ray Observatory. July 16, 2009.
- Walter, Frederick M.; Lattimer, James M., The Astrophysical Journal, 2002
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- ↑ "The Mystery of the Lonely Neutron Star"Script error: No such module "Unsubst".. European Southern Observatory press release, September 11, 2000. Accessed online at spaceref.com May 20, 2007.
- ↑ a b Script error: No such module "Citation/CS1".
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