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...age=en|volume=332|issue=3|pages=L65–L68|doi=10.1046/j.1365-8711.2002.05539.x|arxiv=astro-ph/0206365 |issn=0035-8711|bibcode=2002MNRAS.332L..65B|doi-acce ...l|last1=Stelzer|first1=B.|last2=Micela|first2=G.|date=October 2007|title=X-ray detection of the substellar twin 2MASS J11011926-7732383 AB|journal=Astrono ...

...colors of the shock structures discovered in [[x-ray]] by the [[Chandra X-ray Observatory]].}} ...Laura |last4=Aydi |first4=Elias |last5=Sokolovsky |first5=Kirill V. |last6=Ray |first6=Paul S. |last7=Kerr |first7=Matthew |date=2022-12-01 |title=A New F ...

...e="podsiadlowski">{{cite web |url=http://www-astro.physics.ox.ac.uk/~podsi/binaries.pdf |title=The Evolution of Binary Systems, in Accretion Processes in Astro ...623]–665 |chapter=Chapter 16: Formation and evolution of compact stellar X-ray sources |arxiv=astro-ph/0303456 |isbn=978-0-521-82659-4 |name-list-style=am ...

The system is a likely (99.4% chance) source of the [[X-ray astronomy|X-ray emission]] coming from these coordinates.<ref name=Haakonsen2009/> | doi=10.1111/j.1365-2966.2008.13596.x | doi-access=free | postscript=. ...

...tedly for a red giant, Pi Geminorum was found to be an [[X-ray astronomy|X-ray source]] during the [[ROSAT]] all-sky survey. The most likely source for th | doi=10.1111/j.1365-2966.2008.13596.x | doi-access=free | bibcode=2008MNRAS.389..869E ...

| x%=60.6 | y%=35.0 Kappa Fornacis was found to be 0.23 arcseconds north of an [[X-ray]] and [[Radio]] source in 1995, a distance so close that it is most likely ...

| caption = PSR J0952–0607 (center crosshair) imaged by the [[Fermi Gamma-ray Space Telescope]] | names = PSR J0952–0607, [[Fermi Gamma-ray Space Telescope|4FGL]] J0952.1–0607 ...

...eriod is approximately five times the binary orbital period. For eccentric binaries, the period of accretion variability is the same as the binary orbital peri Eccentric binaries also see accretion variability over secular timescales hundreds of times th ...

...weak fields ≲ 10⁹ [[gauss (unit)|G]] (ms pulsars, lowmass X-ray binaries). If these two groups have an evolutionary connection, their dipole moment | doi = 10.1111/j.1365-2966.2006.10667.x ...

...ter Pan disks (J0446, J0949, LDS 5606 and J1915) are binaries or suspected binaries.<ref name="Silverberg2020" /><ref name="Lee2020" /><ref name="Stahl2022" /> ...T Tauri stars. The researchers of this study concluded that the current X-ray luminosity of Peter Pan disk cannot explain their old age. The old age of t ...

...er |first4=Y. |year=2006 |title=Accurate Evolutions of Orbiting Black-Hole Binaries without Excision |journal=Physical Review Letters |volume=96 |issue=11 |pag ...for detection. However, since little was known about the number of compact binaries in the universe and reaching that final stage can be very slow, there was l ...

...rst=Oscar |year=2021 |title=Primordial black hole origin for thermal gamma-ray bursts |journal=Monthly Notices of the Royal Astronomical Society |volume=5 ...rst3=Marc |date=2017-12-19 |title=The merger rate of primordial-black-hole binaries |journal=Physical Review D |volume=96 |issue=12 |pages=123523 |arxiv=1709.0 ...

|x=379|y=719 ...name=gosset/> For comparison, the Sun [[Solar wind#Emission|loses]] (2-3) x 10⁻¹⁴ solar masses per year due to its [[solar wind]], several h ...

...understood as functions of the configuration space coordinates <math>\vec{x},t</math>, ''i.e.'' functions of space and time. Taking the [[Fourier trans :<math>\hat \psi(\vec k) = \int e^{-i\vec k\cdot \vec x}\; \psi(\vec x) \;dx</math> ...

...rises with the time is typical of gravitational waves from compact object binaries, and its exact shape is mainly determined by the masses of the objects.]] ...itive to the late stages of the coalescence of black hole and neutron star binaries: only the last seconds of the whole process can currently be observed (incl ...

| doi=10.1111/j.1365-2966.2010.16253.x| doi-access=free |bibcode = 2010MNRAS.403.1829S | s2cid=118697588 }}</ref> | doi=10.1046/j.1365-8711.1998.01600.x ...

-\frac{\hbar^2}{2m} \frac{\partial^2\Psi(x,t)}{\partial x^2} + V(x,t)\Psi(x,t) &=E\Psi(x,t) ...

...]] |volume=311 |issue=2 |pages=441–447 |doi=10.1046/j.1365-8711.2000.03075.x |doi-access=free |arxiv=astro-ph/9909252 |bibcode = 2000MNRAS.311..441C|s2c ...gravitational) [[mass]], {{mvar|a}} is its acceleration, {{mvar|μ}}({{mvar|x}}) is an as-yet unspecified function (called the ''interpolating function'' ...

...rst9=L. |last10=Stolker |first10=T. |last11=Balmer |first11=W. -O. |last12=Ray |first12=S. |last13=Bonnefoy |first13=M. |last14=Mollière |first14=P. |last ...|first9=Marc |last10=Matsumura |first10=Soko |last11=Jayawardhana |first11=Ray |last12=Chambers |first12=John |last13=Bromley |first13=Ben |year=2013 |tit ...

...hive.today/20231023124510/https://www.nature.com/articles/s41550-023-02101-x |archive-date=23 October 2023 |access-date=23 October 2023 |arxiv=2307.0230 ...}</ref> One FRB seems to have been in the same location as a known [[gamma-ray burst]].<ref name=Wang>{{cite journal |display-authors=etal|last1=Wang |fir ...