PSR J0952–0607

**PSR J0952–0607**
	; 由費米伽馬射線太空望遠鏡成像的PSR J0952–0607（中心十字線）
觀測資料; 曆元 J2000.0
星座	六分儀座
星官
赤經	09h 52m 08.319s
赤緯	−06° 07′ 23.49″
視星等（V）
特性
光谱分类	脈衝星
视星等 (i)	22.0–24.4
天体测定
距离	970+1160; −530 pc; or 1740+1570; −820 pc; or 6260+360; −400 (optical) pc
詳細資料
PSR J0952–0607 A
質量	2.35±0.17 M☉
自轉	1.41379836 ms
年齡	4.9 Gyr
PSR J0952–0607 B
質量	0.032±0.002 M☉
亮度	9.96+1.20; −1.12 L☉
溫度	3085+85; −80 K
	軌道
主星	PSR J0952–0607 A
伴星	PSR J0952–0607 B
繞行週期 (P)	0.267461035 d; (6.41906484 h)
半長軸 (a)	1600000 km
偏心率 (e)	<0.004
倾斜角 (i)	59.8+2.0; −1.9°
半振幅 (K2); (secondary)	376.1±5.1 km/s
其他命名
	PSR J0952–0607, 4FGL J0952.1–0607
參考資料庫
SIMBAD	资料

PSR J0952–0607是雙星系統中的一顆巨大的毫秒脈衝星，位於六分儀座中，距離地球 3,200–5,700 光年（970–1,740 pc）。^[5] 它保持著截至 2022年已知質量最大的中子星的記錄，質量是太陽的 2.35±0.17 倍，可能接近中子星的托爾曼-奧本海默-沃爾科夫質量上限。^[4]^[6] 此脈衝星以 707 Hz（1.41 毫秒週期）的頻率旋轉，使其成為已知旋轉第二快的脈衝星，也是銀河系內已知旋轉最快的脈衝星。^[7]^[5]

雙星系統[编辑]

藝術家對黑寡婦脈衝星系統的想像畫，其中一個恆星質量伴星正在被其宿主脈衝星的強烈輻射剝離

PSR J0952–0607雙星系統包含一顆質量巨大的脈衝星和一個亞恆星質量（<0.1 太陽質量）^[8]^{（p. 127）}的伴星組成，緊密環繞在其周圍^[4]。由於這種配置，該系統屬於“黑寡婦脈衝星”類型^[6]，這種類型的脈衝星會“吞噬”它們的伴星。伴星因強烈的高能太陽風和脈衝星發出的伽馬射線的侵蝕而不斷失去質量，脈衝星並將伴星失去的物質吸積到自己身上。^[8]^{（p. 127）}^[4]^{（p. 1）}

註釋[编辑]

^ 引证错误：没有为名为luminosity的参考文献提供内容
^ 引证错误：没有为名为semimajor的参考文献提供内容

參考資料[编辑]

^ ^1.0 ^1.1 PSR J0952-0607 -- Pulsar. SIMBAD. Centre de données astronomiques de Strasbourg. [26 July 2022].
^ Draghis, Paul; Romani, Roger W.; Filippenko, Alexei V.; Brink, Thomas G.; Zheng, WeiKang; Halpern, Jules P.; Fernando, Camilo. Multiband Optical Light Curves of Black-widow Pulsars. The Astrophysical Journal. September 2019, 883 (1): 13. Bibcode:2019ApJ...883..108D. arXiv:1908.00992 . doi:10.3847/1538-4357/ab378b . 108.
^ ^3.0 ^3.1 ^3.2 ^3.3 ^3.4 Nieder, L.; Clark, C. J.; Bassa, C. G.; Wu, J.; Singh, A.; Donner, J. Y.; et al. Detection and Timing of Gamma-Ray Pulsations from the 707 Hz Pulsar J0952-0607. The Astrophysical Journal. September 2019, 883 (1): 17. Bibcode:2019ApJ...883...42N. arXiv:1905.11352 . doi:10.3847/1538-4357/ab357e . 42.
^ ^4.0 ^4.1 ^4.2 ^4.3 ^4.4 ^4.5 ^4.6 ^4.7 Romani, Roger W.; Kandel, D.; Filippenko, Alexei V.; Brink, Thomas G.; Zheng, WeiKang. PSR J0952-0607: The Fastest and Heaviest Known Galactic Neutron Star. The Astrophysical Journal Letters. August 2022, 934 (2): 6. Bibcode:2022ApJ...934L..17R. arXiv:2207.05124 . doi:10.3847/2041-8213/ac8007 . L18.
^ ^5.0 ^5.1 Reddy, Francis. 'Extreme' Telescopes Find the Second-fastest-spinning Pulsar. NASA. 5 September 2017 [26 July 2022].
^ ^6.0 ^6.1 Sanders, Robert. Heaviest neutron star to date is a 'black widow' eating its mate. Berkeley News (University of California Berkeley). 26 July 2022 [26 July 2022].
^ Bassa, C. G.; Pleunis, Z.; Hessels, J. W. T.; Ferrara, E. C.; Breton, R. P.; Gusinskaia, N. V.; et al. LOFAR Discovery of the Fastest-spinning Millisecond Pulsar in the Galactic Field. The Astrophysical Journal Letters. September 2017, 846 (2): 7. Bibcode:2017ApJ...846L..20B. arXiv:1709.01453 . doi:10.3847/2041-8213/aa8400 . L20.
^ ^8.0 ^8.1 Roberts, Mallory S. E. Surrounded by spiders! New black widows and redbacks in the Galactic field. Proceedings of the International Astronomical Union. March 2013, 291: 127–132. Bibcode:2013IAUS..291..127R. arXiv:1210.6903 . doi:10.1017/S174392131202337X .

引证错误：在<references>标签中name属性为“Mukherjee2017”的参考文献没有在文中使用
引证错误：在<references>标签中name属性为“Ho2019”的参考文献没有在文中使用
引证错误：在<references>标签中name属性为“Abdollahi2020”的参考文献没有在文中使用
引证错误：在<references>标签中name属性为“Kohler2019”的参考文献没有在文中使用

引证错误：在<references>标签中name属性为“ScienceAlert2019”的参考文献没有在文中使用

Template:2022 in space Template:Sextans

[luminosity-5] 引证错误：没有为名为luminosity的参考文献提供内容

[semimajor-6] 引证错误：没有为名为semimajor的参考文献提供内容

[Simbad-1] 1.0 ^1.1 PSR J0952-0607 -- Pulsar. SIMBAD. Centre de données astronomiques de Strasbourg. [26 July 2022].

[Draghis2019-2] Draghis, Paul; Romani, Roger W.; Filippenko, Alexei V.; Brink, Thomas G.; Zheng, WeiKang; Halpern, Jules P.; Fernando, Camilo. Multiband Optical Light Curves of Black-widow Pulsars. The Astrophysical Journal. September 2019, 883 (1): 13. Bibcode:2019ApJ...883..108D. arXiv:1908.00992 . doi:10.3847/1538-4357/ab378b . 108.

[Nieder2019-3] 3.0 ^3.1 ^3.2 ^3.3 ^3.4 Nieder, L.; Clark, C. J.; Bassa, C. G.; Wu, J.; Singh, A.; Donner, J. Y.; et al. Detection and Timing of Gamma-Ray Pulsations from the 707 Hz Pulsar J0952-0607. The Astrophysical Journal. September 2019, 883 (1): 17. Bibcode:2019ApJ...883...42N. arXiv:1905.11352 . doi:10.3847/1538-4357/ab357e . 42.

[Romani2022-4] 4.0 ^4.1 ^4.2 ^4.3 ^4.4 ^4.5 ^4.6 ^4.7 Romani, Roger W.; Kandel, D.; Filippenko, Alexei V.; Brink, Thomas G.; Zheng, WeiKang. PSR J0952-0607: The Fastest and Heaviest Known Galactic Neutron Star. The Astrophysical Journal Letters. August 2022, 934 (2): 6. Bibcode:2022ApJ...934L..17R. arXiv:2207.05124 . doi:10.3847/2041-8213/ac8007 . L18.

[NASA2017-7] 5.0 ^5.1 Reddy, Francis. 'Extreme' Telescopes Find the Second-fastest-spinning Pulsar. NASA. 5 September 2017 [26 July 2022].

[Berkeley-8] 6.0 ^6.1 Sanders, Robert. Heaviest neutron star to date is a 'black widow' eating its mate. Berkeley News (University of California Berkeley). 26 July 2022 [26 July 2022].

[Bassa2017-9] Bassa, C. G.; Pleunis, Z.; Hessels, J. W. T.; Ferrara, E. C.; Breton, R. P.; Gusinskaia, N. V.; et al. LOFAR Discovery of the Fastest-spinning Millisecond Pulsar in the Galactic Field. The Astrophysical Journal Letters. September 2017, 846 (2): 7. Bibcode:2017ApJ...846L..20B. arXiv:1709.01453 . doi:10.3847/2041-8213/aa8400 . L20.

[Roberts2013-10] 8.0 ^8.1 Roberts, Mallory S. E. Surrounded by spiders! New black widows and redbacks in the Galactic field. Proceedings of the International Astronomical Union. March 2013, 291: 127–132. Bibcode:2013IAUS..291..127R. arXiv:1210.6903 . doi:10.1017/S174392131202337X .

[1]

[2]

[3]

[4]

[a]

[b]

[5]

[6]

[7]

[8]