PSR B0950+08

PSR B0950+08
Observation data; Epoch J2000 Equinox J2000
Constellation	Leo
Right ascension	09h 53m 09.310s
Declination	+07° 55' 35.75"'
Apparent magnitude (V)	5.28
Characteristics
Variable type	Pulsar
Astrometry
Proper motion (μ)	RA: -2.09 mas/yr ; Dec.: 29.46 mas/yr
Parallax (π)	3.82 ± 0.07 mas
Distance	850 ± 20 ly ; (262 ± 5 pc)
Details
Age	1.8 million years
Other designations
	PSR J0953+0755, NVSS J095309+075536, 0950, 228.9+43.7, PSR B0950+08.
Database references
SIMBAD	data

Coordinates: 09^h 53^m 09.310^s, +07° 55′ 35.75″

PSR B0950+08 is a young pulsar that may have come from a supernova that occurred in Leo 1.8 million years ago. The remnant of this supernova may be the nearest besides the Local Bubble, and the supernova would have been as bright as the moon. Off-pulse emissions from the young pulsar were detected by the Expanded Long Wavelength Array, suggesting the presence of a pulsar wind nebula around it.^[1]

External links[]

References[]

^ Ruan, D. (8 May 2020). "Discovery of a Pulsar Wind Nebula around B0950+08 with the ELWA". Monthly Notices of the Royal Astronomical Society. arXiv:2005.03303. doi:10.1093/mnras/staa1305. S2CID 218537942.

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[Ruan2020-1] Ruan, D. (8 May 2020). "Discovery of a Pulsar Wind Nebula around B0950+08 with the ELWA". Monthly Notices of the Royal Astronomical Society. arXiv:2005.03303. doi:10.1093/mnras/staa1305. S2CID 218537942.

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