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...vered as of January 2011. Three of them are Intermittent millisecond X-ray pulsars (HETE J1900.1-2455, Aql X-1 and SAX J1748.9-2021), i.e. they emit pulsation ...irst9=S. R. |last10=Depoy |first10=D. L. |last11=Hakala |first11=P. |title=Optical spectroscopy and photometry of SAX J1808.4-3658 in outburst |journal=Monthl ...

| title = About Pulsars ...y pulsar]]s, which are mostly [[magnetar]]s. Some radio pulsars are also [[optical pulsar]]s. ...

PSR B0950+08 was fourth among the initial [[radio pulsars]] discovered in 1968.<ref name="Zharikov2002"/> <ref name="Zharikov2002">{{cite journal | title=Subaru optical observations of the old pulsar PSR B0950+08 | last1=Zharikov | first1=S. V. ...

* The [[Cambridge Optical Aperture Synthesis Telescope|Cambridge Optical Aperture Synthesis Telescope (COAST)]] ...rious [[Aperture Masking Interferometry|aperture masking]] instruments for optical [[aperture synthesis]] ...

...with the red star in the centre being the [[Crab Pulsar]]. Image combines optical data from [[Hubble Space Telescope|Hubble]] (in red) and [[X-ray astronomy| ...s.<ref name="Weiler1978" /> They have since been found to be [[infrared]], optical, millimetre, [[X-ray]]<ref name="SafiHarb2012">{{cite conference |title=Ple ...

* [[Pulsar|Pulsars]] ===Atmospheric optical phenomena=== ...

...al wave]] signal [[GW170817]], short [[gamma-ray bursts]] [[GRB 170817A]], optical transient [[AT 2017gfo]] and other electromagnetic signals.<ref name="PhysR ...

The '''Vela Pulsar''' (PSR J0835-4510 or PSR B0833-45) is a radio, optical, [[X-ray]]- and [[Gamma ray|gamma]]-emitting [[pulsar]] associated with the [[File:HUVelLightCurve.png|thumb|left|[[Gamma ray]] and optical (visible light) [[light curve]]s for the pulsar, adapted from Spolon et al. ...

*Pulsars *Millisecond Pulsars, ...

...red by a number of independent methods. The proper motion of the expanding optical shell of 3C 58 has been measured three times, always with an indicated age | title=Optical Imaging and Spectroscopy of the Galactic Supernova Remnant 3C 58 (G130.7+3. ...

...p;metres and 15&nbsp;metres in [[diameter]], as well as the largest Polish optical telescope – 90&nbsp;cm Schmidt-Cassegrain camera. The facility is operated ...o galaxies]] and [[quasars]], [[observational cosmology]], the timing of [[pulsars]], the search for new [[planetary systems]] and [[Solar System]] studies. I ...

...applications, the brightness temperature of a surface is determined by an optical measurement, for example using a [[pyrometer]], with the intention of deter ...p;K.<ref name="blan92">{{cite journal |last1=Blandford |first1=R.D. |title=Pulsars and Physics |journal=Philosophical Transactions: Physical Sciences and Engi ...

...ipsoidal<ref name=tjemkes>{{cite journal|bibcode=1986A&A...154...77T|title=Optical light curves of massive X-ray binaries|journal=Astronomy and Astrophysics|v ...d in the X-ray band as well as the minimum mass of the occulting star, the optical component remained undiscovered for three years. This was partly because Ce ...

...fore the discovery of [[pulsar]]s), [[Iosif Shklovsky]] examined X-ray and optical observations of Scorpius X-1 and correctly concluded that the radiation com [[File:V818ScoLightCurve.png|thumb|left|A broadband optical [[light curve]] for V818 Scorpii, adapted from Hynes ''et al.'' (2016)<ref ...

...ation |last1=Patruno |first1=Alessandro |title=Accreting Millisecond X-ray Pulsars |date=2021 |url=https://doi.org/10.1007/978-3-662-62110-3_4 |work=Timing Ne ...te journal |bibcode = 2000ApJ...530L..93T|title = Formation of Millisecond Pulsars with Heavy White Dwarf Companions:Extreme Mass Transfer on Subthermal Times ...

...gamma repeater|soft gamma-ray repeaters]], the [[interstellar medium]], [[pulsars]], [[Astrophysical maser|masers]], and [[supernova remnants]]. To the publi ...| author8=Frontera, F. | title=Spectral constraints on the redshift of the optical counterpart to the γ-ray burst of 8 May 1997 | journal=Nature | year=1997 | ...

...hich contains the Crab Pulsar (the red star in the center). Image combines optical data from [[Hubble Space Telescope|Hubble]] (in red) and X-ray images from | appmag_v=16.65<ref>{{citation|title=Optical Observations of Pulsars: the ESO Contribution |page=22|url=https://www.eso.org/sci/publications/mes ...

.../2011/03/25/a-pulsar-alone/|title=A Pulsar Alone: The first deep X-ray and optical observations of the closest isolated radio pulsar|last=Kohler|first=Susanna [[Category:Rotation-powered pulsars]] ...

...983"/> The characteristics of the x-ray source were unique: large x-ray to optical luminosity, no radio emission detected by the sensitive [[Very Large Array| ...">{{cite journal |last1=Mignani |first1=Roberto P. |date=April 2011 |title=Optical, ultraviolet, and infrared observations of isolated neutron stars |journal= ...

.... M. | last5=Freire | first5=P. C. C. | title=A 1.4 GHz Arecibo Survey for Pulsars in Globular Clusters | journal=The Astrophysical Journal | volume=670 | iss ...7=Freire | first7=P. C. | last8=Belczynski | first8=K. | title=Young Radio Pulsars in Galactic Globular Clusters | journal=The Astrophysical Journal | volume= ...