Astronomy:PSR J1928+1815
240px Diagram showing the common envelope phase. | |
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Sagitta[1] |
| Right ascension | 19h 28m 08.3490s |
| Declination | +18° 15′ 30.270″ |
| Astrometry | |
| Distance | 455 ly (139 pc) |
| Details | |
| Mass | 1.44 M☉ |
| Rotation | 10.5494989888508 ms |
| Age | 46 Myr |
| Other designations | |
PSR J1928+1815 | |
| Database references | |
| SIMBAD | data |
PSR J1928+1815 is a millisecond pulsar located 455 light years (139 parsecs) from Earth with a rotation period of 10.549 milliseconds and is characteristic age of 46 million years old. It is in a 3.6 hour long binary orbit with a helium-dominated star with 1.0–1.6 solar masses that recently went through a red giant phase.[2][3]
Theoretical models have shown that relatively recently, the helium star which was then a main sequence star expanded into a red giant star engulfing PSR J1928+1815 within its outer envelope layers. After several thousand years, the outer envelope was ejected into space and some mass was transferred to the millisecond pulsar increasing its spin rate.[2] This binary system has scientific value since while models predict that binary stars will likely have one star orbiting within the expanded envelope of the other dying star, it has not been observed. It is estimated that there are around 16 to 84 of theses stars located somewhere in the Milky Way galaxy with the PSR J1928+1815 binary system being one of them.[4][5]
References
- ↑ Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific 99 (617): 695. doi:10.1086/132034. Bibcode: 1987PASP...99..695R Constellation record for this object at VizieR.
- ↑ 2.0 2.1 Yang, Z. L.; Han, J. L.; Zhou, D. J.; Jing, W. C.; Chen, W. C.; Wang, T.; Li, X. D.; Wang, S. et al. (22 May 2025). "A pulsar-helium star compact binary system formed by common envelope evolution". Science 388 (6749): 859–863. doi:10.1126/science.ado0769. PMID 40403072. Bibcode: 2025Sci...388..859Y. https://www.science.org/doi/10.1126/science.ado0769.
- ↑ "Scientists find rare double-star system where one star orbited inside the other" (in en). 22 May 2025. https://www.space.com/astronomy/stars/scientists-find-rare-double-star-system-where-one-star-orbited-inside-the-other.
- ↑ "Newly-Discovered Compact Binary System Formed when Neutron Star Orbited inside Another Star | Sci.News" (in en-US). 22 May 2025. https://www.sci.news/astronomy/pulsar-helium-star-compact-binary-system-13932.html.
- ↑ "Rare binary star system formed when a neutron star orbited inside another star" (in en). https://www.eurekalert.org/news-releases/1084285.
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