J1713+0747
(binary system with millisecond pulsar and white dwarf)
J1713+0747 is a binary star consisting of a
millisecond pulsar (MSP) (PSR J1713+0747)
and a white dwarf, discovered in the early 1990s
in Arecibo Observatory pulsar searches.
It has been used for study due to its high consistency.
The pulsar is one of NANOGrav's observed MSPs.
(star,pulsar,neutron star,binary star,white dwarf)
Further reading:
https://ui.adsabs.harvard.edu/abs/1994ApJ...437L..39C/abstract
https://ui.adsabs.harvard.edu/abs/2005ApJ...620..405S/abstract
https://ui.adsabs.harvard.edu/abs/2015ApJ...809...41Z/abstract
http://simbad.u-strasbg.fr/simbad/sim-id?Ident=PSR%20J1713%2B0747
| Redshift | Parsecs
/Distance | Lightyears
/Lookback Years | | |
| ~0 | 1.15kpc | 3.75kly | | J1713+0747 |
|
| Coordinates: | J1713+0747
J171349.53053+074737.5264 |
|
Referenced by page:
rotation period
Index