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- | rotation=2.5 [[millisecond|ms]]<ref name="Pletsch2012">[[#Pletsch2012|Pletsch et al. (2012)]]</ref> ...is a [[pulsar]] with a spin period of 2.5 milliseconds. It is the first [[millisecond pulsar]] found via gamma-ray pulsations. The source was originally identifi ...10 KB (1,467 words) - 20:42, 21 January 2024
- ...Flaring Black Widow Candidate and Demographics of Black Widow Millisecond Pulsars in the Galactic Field |journal=The Astrophysical Journal |volume=941 |issue ...=https://www.aei.mpg.de/830748/gamma-ray-eclipses-shed-new-light-on-spider-pulsars |access-date=2023-01-27 |website=www.aei.mpg.de |language=en}}</ref> ...8 KB (1,140 words) - 06:20, 22 December 2023
- {{Short description|Millisecond pulsar in the constellation Serpens}} | class = [[millisecond pulsar]]<ref name=bailes/> <!--Stellar class--> ...10 KB (1,463 words) - 14:07, 9 December 2024
- ...lue points with error bars represent the results from correlating pairs of pulsars. (GWB = gravitational wave background).<ref name=":1">{{Cite web |title=Evi ...te=2023-08-24 |title=Hellings and Downs correlation of an arbitrary set of pulsars |url=https://link.aps.org/doi/10.1103/PhysRevD.108.043026 |journal=Physical ...13 KB (1,741 words) - 00:25, 14 July 2024
- ...eleration of charged particles in the light cylinder area of the Crab-like pulsars. It has been shown that electrons might achieve the Lorentz factors <math>\ ...im|first2 = K.|bibcode = 2008PhPl...15c2901O|s2cid = 119330230}}</ref> and pulsars.<ref>{{Cite arXiv |eprint = astro-ph/0609383|last1 = Rieger|first1 = F. M.| ...12 KB (1,654 words) - 05:24, 5 January 2025
- | rotation= 39.1226569017806 [[millisecond|ms]]<ref name="Antoniadis2013"/> ...cope]]s that operate in the [[gamma ray]] wavelengths have also discovered pulsars. ...12 KB (1,544 words) - 02:29, 30 July 2024
- {{Short description|Massive millisecond pulsar in the Milky Way}} ...keley"/> The [[pulsar]] rotates at a frequency of 707 [[Hertz|Hz]] (1.41 [[millisecond|ms]] period), making it the second-fastest-spinning pulsar known, and the f ...20 KB (2,452 words) - 19:52, 26 December 2024
- ...be better sampled by many more pulsar pairings. With such a GW detection, millisecond pulsar timing arrays would open a new low-frequency window in [[gravitation [[File:Pulsar-timing-array-schematic.svg|thumb|upright=1.5|The pulsars P1 ... Pn are sending signals periodically, which are received on Earth. A ...24 KB (3,232 words) - 23:38, 22 February 2025
- ...ve an evolutionary connection, their dipole moment must decay. Millisecond pulsars are believed to have been spun up to their fast rotation by accretion from ...11 KB (1,522 words) - 16:56, 19 January 2025
- ...es of young isolated neutron stars which are different from standard radio pulsars, such as [[soft gamma repeater]]s, [[anomalous X-ray pulsar]]s, [[rotating ...tron stars]] with a galactic birth rate larger than that of normal [[radio pulsars]]. ...16 KB (2,181 words) - 18:43, 26 December 2024
- ...=10.1126/science.1208890|title=Transformation of a Star into a Planet in a Millisecond Pulsar Binary| year=2011| last1=Bailes|first1=M.|author1-link=Matthew Baile ...8/355145a0 |s2cid=4260368}}</ref> Another example is [[PSR J1719-1438]], a millisecond pulsar whose companion, [[PSR J1719-1438 b]], has a minimum mass approximat ...19 KB (2,663 words) - 21:32, 18 July 2024
- ...s discovered by [[radio astronomer]]s on 19 July 2017, during a survey for pulsars with the [[Arecibo Observatory]]'s {{convert|305|m|ft|adj=on|sigfig=3}} rad ...by [[radio astronomer]]s on 19 July 2017, during the [[PALFA Survey]] for pulsars in the [[Milky Way]]'s [[galactic plane]] with the [[Arecibo Observatory]]' ...20 KB (2,633 words) - 17:15, 18 July 2024
- ...RAX array expects to detect tens of FRBs per day.<ref name = newburgh15 /> Pulsars are rapidly rotating [[neutron stars]], whose rotation causes them to appea ...15 KB (2,207 words) - 13:17, 2 June 2024
- ...erstood. Astronomers estimate the average FRB releases as much energy in a millisecond as the Sun puts out in three days.<ref>{{Cite journal|last1=Petroff|first1= ...wn.<ref>{{cite web |last1=Scholz |first1=Paul |title=ATel #13681: A bright millisecond-timescale radio burst from the direction of the Galactic magnetar SGR 1935+ ...155 KB (20,398 words) - 06:38, 23 February 2025
- ...t4=Wei|first4=Y. C.|last5=Li|first5=X. D.|date=October 2007|title=Does Sub-millisecond Pulsar XTE J1739-285 Contain a Low Magnetic Neutron Star or Quark Star ?|jo ...mating the dark matter halo velocity and surface temperature of some known pulsars due to dark matter capture|class=hep-ph |eprint=2402.13795}}</ref> ...149 KB (20,469 words) - 03:47, 17 February 2025