RX J1856.5−3754

From Wikipedia the free encyclopedia

RX J1856.5−3754

X-ray image of RX J1856.5−3754
Observation data
Epoch 1996.7      Equinox J2000.0[1]
Constellation Corona Australis
Right ascension 18h 56m 35s[1]
Declination −37° 54′ 36″[1]
Apparent magnitude (V) ~25.6[1]
Details
Mass0.9 M☉
Radius19–41 km
Age1 Myr
Other designations
RX J185635−3754, 1ES 1853−37.9, 1RXS J185635.1−375433
Database references
SIMBADdata

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

[edit]
Zooming in on the very faint neutron star RX J1856.5–3754
Hubble image of RX J1856.5−3754—the first direct observation of an isolated neutron star in visible light

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 108 km/s. It was discovered in 1992, and observations in 1996 confirmed that it is a neutron star, the closest to Earth discovered to date.[2]

It was originally thought to be about 150–200 light-years away,[3] but further observations using the Chandra X-ray Observatory in 2002 indicate that its distance is greater—about 400 light-years.[4][5]

RX J1856 is one of the Magnificent Seven, a group of young neutron stars at distances between 130 and 500 parsecs (420 and 1,630 light-years) of Earth.

Quark star hypothesis

[edit]

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 700,000 °C and has a diameter of about 4–8 km. 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.[4]

However, later refined analysis[5][6] of improved Chandra and Hubble observations revealed that the surface temperature of the star is lower, only 434,000 °C, and, respectively, the diameter is larger, about 14 km (with account of the effects of general relativity, the observed radius appears about 17 km).[5] Thus, RX J1856.5–3754 is now excluded from the list of quark star candidates.[6]

Vacuum birefringence

[edit]
The polarization of the observed light in the extremely strong magnetic field suggests that the empty space around the neutron star is subject to the vacuum birefringence.[7]

In 2016 a team of astronomers from Italy, Poland, and the U.K. using the Very Large Telescope reported[8][9] 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.[10]

Its inferred magnetic effect of 1013 G should produce a greater effect at X-ray wavelength 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).[11]

See also

[edit]
  • 3C 58, a possible quark star

References

[edit]
  1. ^ a b c d F. M. Walter. "RX J185635-3754 - an Isolated Neutron Star". Department of Physics and Astronomy, State University of New York at Stony Brook. Retrieved June 29, 2007.
  2. ^ Rees, Martin (2012). Universe. Dorling Kindersley. p. 528. ISBN 978-1-4093-7650-7.
  3. ^ "The Mystery of the Lonely Neutron Star". European Southern Observatory press release, September 11, 2000. Accessed online at spaceref.com May 20, 2007.
  4. ^ a b Drake J. J.; et al. (2002). "Is RX J1856.5-3754 a Quark Star?". Astrophys. J. 572 (2): 996–1001. arXiv:astro-ph/0204159. Bibcode:2002ApJ...572..996D. doi:10.1086/340368. S2CID 18481546.
  5. ^ a b c Ho W. C. G.; et al. (2007). "Magnetic hydrogen atmosphere models and the neutron star RX J1856.5–3754". Monthly Notices of the Royal Astronomical Society. 375 (2): 821–830. arXiv:astro-ph/0612145v1. Bibcode:2007MNRAS.375..821H. doi:10.1111/j.1365-2966.2006.11376.x. S2CID 2046995.
  6. ^ a b Truemper, J. E.; Burwitz, V.; Haberl, F.; Zavlin, V. E. (June 2004). "The puzzles of RX J1856.5-3754: neutron star or quark star?". Nuclear Physics B: Proceedings Supplements. 132: 560–565. arXiv:astro-ph/0312600. Bibcode:2004NuPhS.132..560T. doi:10.1016/j.nuclphysbps.2004.04.094. S2CID 425112.
  7. ^ "First Signs of Weird Quantum Property of Empty Space? – VLT observations of neutron star may confirm 80-year-old prediction about the vacuum". www.eso.org. Retrieved 5 December 2016.
  8. ^ Mignani, R. P.; Testa, V.; González Caniulef, D.; Taverna, R.; Turolla, R.; Zane, S.; Wu, K. (2016-11-02). "Evidence for vacuum birefringence from the first optical-polarimetry measurement of the isolated neutron star RX J1856.5−3754". Monthly Notices of the Royal Astronomical Society. 465 (1). Oxford University Press (OUP): 492–500. arXiv:1610.08323. doi:10.1093/mnras/stw2798. ISSN 0035-8711.
  9. ^ "Astronomers Report First Observational Evidence for Vacuum Birefringence | Astronomy | Sci-News.com". Breaking Science News | Sci-News.com. Retrieved 2021-10-10.
  10. ^ Fan, Xing; Kamioka, Shusei; Inada, Toshiaki; Yamazaki, Takayuki; Namba, Toshio; et al. (2017). "The OVAL experiment: a new experiment to measure vacuum magnetic birefringence using high repetition pulsed magnets". The European Physical Journal D. 71 (11). Springer Nature: 308. arXiv:1705.00495. Bibcode:2017EPJD...71..308F. doi:10.1140/epjd/e2017-80290-7. ISSN 1434-6060. S2CID 254140737.
  11. ^ "Does This Neutron Star Confirm an 80-Year-Old Quantum Prediction?". Sky & Telescope. 2016-12-07. Retrieved 2021-10-10.
[edit]
Wikimedia Commons has media related to RX J1856.5-3754.
Retrieved from "https://en.wikipedia.org/w/index.php?title=RX_J1856.5−3754&oldid=1245298309"