astro.wikisort.org - Planet
4U 0142+61 is a magnetar at an approximate distance of 13000 light-years from Earth, located in the constellation Cassiopeia.
 | This article includes a list of general references, but it lacks sufficient corresponding inline citations. (May 2017) |
 Artist's conception of 4U 0142+61 | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Cassiopeia |
| Right ascension | 01 46 22.41s |
| Declination | + 61° 45' 03.2" |
| Apparent magnitude (V) | 25.62 |
| Characteristics | |
| B−V color index | 0.63 |
| Variable type | Suspected |
| Astrometry | |
| Proper motion (μ) | RA: 26.58958 mas/yr Dec.: +61.75264 mas/yr |
| Details | |
| Luminosity | 0.63 L☉ |
| Rotation | 8.68832905 s |
| Age | ? years |
| Other designations | |
PSR J0146+61, 1RXS J014621.5+614509 | |
| Database references | |
| SIMBAD | data |
In an article published in Nature on April 6, 2006, Deepto Chakrabarty et al. of MIT revealed that a circumstellar disk was discovered around the pulsar. This may prove that pulsar planets are common around neutron stars. The debris disk is likely to be composed of mainly heavier metals. The star had undergone a supernova event approximately 100,000 years ago. The disk orbits about 1.6 million kilometers away from the pulsar and probably contains about 10 Earth-masses of material.[1] This also marks the first time that a pulsar has been discovered with a debris disk orbiting it.[2]
In May 2022 the first study of IXPE has hinted the possibility of vacuum birefringence on 4U 0142+61[3][4]
References
- Wang, Zhongxiang; Chakrabarty, Deepto; Kaplan, David L. (April 2006). "A debris disk around an isolated young neutron star". Nature. 440 (7085): 772–775. arXiv:astro-ph/0604076. Bibcode:2006Natur.440..772W. doi:10.1038/nature04669. ISSN 0028-0836. PMID 16598251. S2CID 4372235.
- Ertan, Ü; Erkut, M. H.; Ekşi, K. Y.; Alpar, M. A. (March 2007). "The Anomalous X-Ray Pulsar 4U 0142+61: A Neutron Star with a Gaseous Fallback Disk". The Astrophysical Journal. 657 (1): 441–447. arXiv:astro-ph/0612587. Bibcode:2007ApJ...657..441E. doi:10.1086/510303. S2CID 16726942.
- Taverna, Roberto; Turolla, Roberto; Muleri, Fabio; Heyl, Jeremy; Zane, Silvia; Baldini, Luca; Caniulef, Denis González; Bachetti, Matteo; Rankin, John; Caiazzo, Ilaria; Di Lalla, Niccolò; Doroshenko, Victor; Errando, Manel; Gau, Ephraim; Kırmızıbayrak, Demet (2022-05-18). "Polarized x-rays from a magnetar". arXiv:2205.08898 [astro-ph.HE].
- "X-ray polarisation probes extreme physics". CERN Courier. 2022-06-30. Retrieved 2022-08-15.
- Scientists crack mystery of planet formation (April 5, 2006) CNN
- Spitzer Sees New Planet Disk Around Dead Star (April 7, 2006) SpaceDaily
- Birth of 'Phoenix' Planets?
- 4U0142+61
- 1RXS J014621.5+614509
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На других языках
- [en] 4U 0142+61
[es] 4U 0142+61
4U 0142+61 (PSR J0146+61 / 1RXS J014621.5+614509) es un púlsar situado en la constelación de Casiopea con un período de rotación de 8,69 segundos. Se encuentra a 13 000 años luz de distancia del sistema solar. En 2006 se descubrió un disco circunestelar alrededor de este objeto.[1]Другой контент может иметь иную лицензию. Перед использованием материалов сайта WikiSort.org внимательно изучите правила лицензирования конкретных элементов наполнения сайта.
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