Faster access than browser!Similarities between PSR B1937+21 and Pulsar
PSR B1937+21 and Pulsar have 35 things in common (in Unionpedia): Accretion (astrophysics), Aleksander Wolszczan, Angular momentum, Astronomer, Atomic clock, Atomic nucleus, Binary star, Crab Pulsar, Declination, Density, Donald C. Backer, Electromagnetic radiation, Ephemeris time, Franco Pacini, Gravitational wave, Ivor Robinson (physicist), Jocelyn Bell Burnell, Joseph Hooton Taylor Jr., Millisecond, Millisecond pulsar, Monthly Notices of the Royal Astronomical Society, Neutron star, Plasma (physics), PSR B1257+12, PSR B1919+21, PSR J1748-2446ad, Radio wave, Right ascension, Russell Alan Hulse, Star, ..., Sun, Supernova remnant, Thomas Gold, Wavelength, X-ray. Expand index (5 more) »
Accretion (astrophysics)
In astrophysics, accretion is the accumulation of particles into a massive object by gravitationally attracting more matter, typically gaseous matter, in an accretion disk.
Accretion (astrophysics) and PSR B1937+21 · Accretion (astrophysics) and Pulsar ·
Aleksander Wolszczan
Aleksander Wolszczan (born 29 April 1946 in Szczecinek, Poland) is a Polish astronomer.
Aleksander Wolszczan and PSR B1937+21 · Aleksander Wolszczan and Pulsar ·
Angular momentum
In physics, angular momentum (rarely, moment of momentum or rotational momentum) is the rotational equivalent of linear momentum.
Angular momentum and PSR B1937+21 · Angular momentum and Pulsar ·
Astronomer
An astronomer is a scientist in the field of astronomy who concentrates their studies on a specific question or field outside the scope of Earth.
Astronomer and PSR B1937+21 · Astronomer and Pulsar ·
Atomic clock
An atomic clock is a clock device that uses an electron transition frequency in the microwave, optical, or ultraviolet region of the electromagnetic spectrum of atoms as a frequency standard for its timekeeping element.
Atomic clock and PSR B1937+21 · Atomic clock and Pulsar ·
Atomic nucleus
The atomic nucleus is the small, dense region consisting of protons and neutrons at the center of an atom, discovered in 1911 by Ernest Rutherford based on the 1909 Geiger–Marsden gold foil experiment.
Atomic nucleus and PSR B1937+21 · Atomic nucleus and Pulsar ·
Binary star
A binary star is a star system consisting of two stars orbiting around their common barycenter.
Binary star and PSR B1937+21 · Binary star and Pulsar ·
Crab Pulsar
The Crab Pulsar (PSR B0531+21) is a relatively young neutron star.
Crab Pulsar and PSR B1937+21 · Crab Pulsar and Pulsar ·
Declination
In astronomy, declination (abbreviated dec; symbol δ) is one of the two angles that locate a point on the celestial sphere in the equatorial coordinate system, the other being hour angle.
Declination and PSR B1937+21 · Declination and Pulsar ·
Density
The density, or more precisely, the volumetric mass density, of a substance is its mass per unit volume.
Density and PSR B1937+21 · Density and Pulsar ·
Donald C. Backer
Donald C. Backer (November 9, 1943 – July 25, 2010) was an American astrophysicist who primarily worked in radio astronomy.
Donald C. Backer and PSR B1937+21 · Donald C. Backer and Pulsar ·
Electromagnetic radiation
In physics, electromagnetic radiation (EM radiation or EMR) refers to the waves (or their quanta, photons) of the electromagnetic field, propagating (radiating) through space-time, carrying electromagnetic radiant energy.
Electromagnetic radiation and PSR B1937+21 · Electromagnetic radiation and Pulsar ·
Ephemeris time
The term ephemeris time (often abbreviated ET) can in principle refer to time in connection with any astronomical ephemeris.
Ephemeris time and PSR B1937+21 · Ephemeris time and Pulsar ·
Franco Pacini
Franco Pacini (May 10, 1939 – January 25, 2012) was an Italian astrophysicist and professor at the University of Florence.
Franco Pacini and PSR B1937+21 · Franco Pacini and Pulsar ·
Gravitational wave
Gravitational waves are the disturbance in the fabric ("curvature") of spacetime generated by accelerated masses and propagate as waves outward from their source at the speed of light.
Gravitational wave and PSR B1937+21 · Gravitational wave and Pulsar ·
Ivor Robinson (physicist)
Ivor Robinson (1923 – May 27, 2016) was an American mathematical physicist, born and educated in England.
Ivor Robinson (physicist) and PSR B1937+21 · Ivor Robinson (physicist) and Pulsar ·
Jocelyn Bell Burnell
Dame Susan Jocelyn Bell Burnell (born 15 July 1943) is an astrophysicist from Northern Ireland who was credited with "one of the most significant scientific achievements of the 20th Century".
Jocelyn Bell Burnell and PSR B1937+21 · Jocelyn Bell Burnell and Pulsar ·
Joseph Hooton Taylor Jr.
Joseph Hooton Taylor Jr. (born March 29, 1941) is an American astrophysicist and Nobel Prize in Physics laureate for his discovery with Russell Alan Hulse of a "new type of pulsar, a discovery that has opened up new possibilities for the study of gravitation.".
Joseph Hooton Taylor Jr. and PSR B1937+21 · Joseph Hooton Taylor Jr. and Pulsar ·
Millisecond
A millisecond (from milli- and second; symbol: ms) is a thousandth (0.001 or 10−3 or 1/1000) of a second.
Millisecond and PSR B1937+21 · Millisecond and Pulsar ·
Millisecond pulsar
A millisecond pulsar (MSP) is a pulsar with a rotational period in the range of about 1–10 milliseconds.
Millisecond pulsar and PSR B1937+21 · Millisecond pulsar and Pulsar ·
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society (MNRAS) is a peer-reviewed scientific journal covering research in astronomy and astrophysics.
Monthly Notices of the Royal Astronomical Society and PSR B1937+21 · Monthly Notices of the Royal Astronomical Society and Pulsar ·
Neutron star
A neutron star is the collapsed core of a large star which before collapse had a total of between 10 and 29 solar masses.
Neutron star and PSR B1937+21 · Neutron star and Pulsar ·
Plasma (physics)
Plasma (Henry George Liddell, Robert Scott, A Greek English Lexicon, on Perseus) is one of the four fundamental states of matter, and was first described by chemist Irving Langmuir in the 1920s.
PSR B1937+21 and Plasma (physics) · Plasma (physics) and Pulsar ·
PSR B1257+12
PSR B1257+12, previously designated PSR 1257+12, alternatively designated PSR J1300+1240, also named Lich, is a pulsar located 2,300 light years from the Sun in the constellation of Virgo.
PSR B1257+12 and PSR B1937+21 · PSR B1257+12 and Pulsar ·
PSR B1919+21
PSR B1919+21 is a pulsar with a period of 1.3373 seconds and a pulse width of 0.04 seconds.
PSR B1919+21 and PSR B1937+21 · PSR B1919+21 and Pulsar ·
PSR J1748-2446ad
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PSR B1937+21 and PSR J1748-2446ad · PSR J1748-2446ad and Pulsar ·
Radio wave
Radio waves are a type of electromagnetic radiation with wavelengths in the electromagnetic spectrum longer than infrared light.
PSR B1937+21 and Radio wave · Pulsar and Radio wave ·
Right ascension
Right ascension (abbreviated RA; symbol) is the angular distance measured only eastward along the celestial equator from the Sun at the March equinox to the (hour circle of the) point above the earth in question.
PSR B1937+21 and Right ascension · Pulsar and Right ascension ·
Russell Alan Hulse
Russell Alan Hulse (born November 28, 1950) is an American physicist and winner of the Nobel Prize in Physics, shared with his thesis advisor Joseph Hooton Taylor Jr., "for the discovery of a new type of pulsar, a discovery that has opened up new possibilities for the study of gravitation".
PSR B1937+21 and Russell Alan Hulse · Pulsar and Russell Alan Hulse ·
Star
A star is type of astronomical object consisting of a luminous spheroid of plasma held together by its own gravity.
PSR B1937+21 and Star · Pulsar and Star ·
Sun
The Sun is the star at the center of the Solar System.
PSR B1937+21 and Sun · Pulsar and Sun ·
Supernova remnant
A supernova remnant (SNR) is the structure resulting from the explosion of a star in a supernova.
PSR B1937+21 and Supernova remnant · Pulsar and Supernova remnant ·
Thomas Gold
Thomas Gold (May 22, 1920June 22, 2004) was an Austrian-born astrophysicist, a professor of astronomy at Cornell University, a member of the U.S. National Academy of Sciences, and a Fellow of the Royal Society (London).
PSR B1937+21 and Thomas Gold · Pulsar and Thomas Gold ·
Wavelength
In physics, the wavelength is the spatial period of a periodic wave—the distance over which the wave's shape repeats.
PSR B1937+21 and Wavelength · Pulsar and Wavelength ·
X-ray
X-rays make up X-radiation, a form of electromagnetic radiation.
The list above answers the following questions
- What PSR B1937+21 and Pulsar have in common
- What are the similarities between PSR B1937+21 and Pulsar
PSR B1937+21 and Pulsar Comparison
PSR B1937+21 has 78 relations, while Pulsar has 134. As they have in common 35, the Jaccard index is 16.51% = 35 / (78 + 134).
References
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