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- determination of a neutron star radius. One method is to study X-ray bursters - these are neutron stars that are still accreting material from a companion in a...3 KB (324 words) - 00:24, 19 September 2019
- X-radiation (composed of X-rays) is a form of electromagnetic radiation. X-rays have a wavelength in the range of 0.01 to 10 nanometers, corresponding...56 KB (7,499 words) - 23:01, 31 January 2024
- Thompson, Duncan (1995) - SGRs as magnetized neutron stars Romani & Yadigaroglu 1995 - gamma-ray pulsars - emission zones and viewing geometries Gil,...12 KB (971 words) - 08:07, 2 November 2015
- actually absorb X-rays and release energy as photons. X-Ray Diffraction measures how light wave reflect off the spacing between atoms, while X-Ray Fluorescence...31 KB (4,517 words) - 21:40, 29 October 2024
- Combinations of w:X-ray images from the Chandra observatory with Hubble's "Pillars" image have shown that X-ray sources (from young stars) do not coincide...4 KB (439 words) - 07:31, 3 September 2018
- rotation-powered radio pulsar and an accretion powered X-ray source. Are all pulsars neutron stars? The answer depends on your definition of a pulsar. Hallinan...10 KB (1,316 words) - 00:17, 30 October 2015
- perspectives. Observations made by w:Chandra X-ray Observatory indicate the presence of loops and rings in the hot X-ray emitting gas that permeate the cluster...8 KB (965 words) - 13:44, 7 September 2009
- for months, and remained visible at night for several years. At X-ray and gamma-ray energies above 30 KeV, the Crab is generally the strongest persistent...4 KB (403 words) - 15:16, 26 November 2012
- radio imaging of the cluster and identified an X-ray source X9 as a new black hole candidate. 300 X-ray sources were detected in the globular cluster by...5 KB (528 words) - 12:01, 17 October 2015
- binary neutron stars or a neutron star with a black hole. The observation of minutes to hours of X-ray flashes after a short gamma-ray burst is consistent...3 KB (420 words) - 14:56, 17 September 2017
- that occur about once every ten years. The w:Chandra X-ray Observatory detected fluctuating w:X-ray emissions from a location approximately 600 light-years...9 KB (956 words) - 13:42, 7 September 2009
- high number of 89 w:variable stars, many of them of the w:RR Lyrae type. The globular also contains a number of w:x-ray sources, thought to be close w:binary...2 KB (141 words) - 13:32, 7 September 2009
- @ SEDS Messier pages 4/10/07: M106 - Mystery Spiral Arms Explained? The X-ray/radio-visible extra spiral arms in M106/NGC 4258. Spiral Galaxy Messier...5 KB (485 words) - 12:47, 19 June 2024
- detected in the galaxy using data from the w:Chandra X-ray Observatory. The black hole, named M33 X-7, orbits a companion star which it eclipses every 3...10 KB (1,272 words) - 10:51, 3 March 2010
- {\displaystyle 2_{1}^{3}H\to \;_{2}^{4}He\;+\;2_{0}^{2}n} 2. In larger stars, carbon-12 ( 6 12 C {\displaystyle _{6}^{12}C} ) is fused with protium (...1 KB (293 words) - 00:14, 31 July 2017
- Contents Instructions and tips for earning the Stars honor can be found in the Nature chapter. The stars appear to move in two different ways. The first...15 KB (4,798 words) - 00:45, 31 July 2017
- holes or w:neutron stars, which are heating incoming gas to millions of kelvins and emitting X-rays. The spectrum of the neutron stars is the same as the...42 KB (5,461 words) - 02:19, 14 August 2014
- zones at high latitudes on the planets. X-rays are higher energy and shorter wavelength than UV. Astronomy in X-rays has specific challenges that do not affect...3 KB (402 words) - 18:03, 1 April 2015
- of a particle of visible light. An X-ray photon will knock the electron right out of an atom, as a result an X-ray can't be generated by electrons transitioning...29 KB (4,866 words) - 01:16, 15 April 2024
- Messier Index/Print Version/1 (section Notable stars)Combinations of w:X-ray images from the Chandra observatory with Hubble's "Pillars" image have shown that X-ray sources (from young stars) do not coincide...778 bytes (6,704 words) - 12:57, 27 July 2010