「PSR」の共起表現一覧(1語右で並び替え)
該当件数 : 77件
| A radome containing Primary Surveillance radar ( | PSR) and Secondary Surveillance Radar (SSR) antenna |
| was associated with the 'Defencist' wing of the | PSR and collaborated closely with V.V. Rudnev, A.R. |
| Cannon remains the publisher of | PSR as of April 2010. |
| The Crab Pulsar ( | PSR B0531+21) is a relatively young neutron star. |
| The pulsar | PSR B0950+08 seems to have come from a supernova th |
| PSR B1257+12 is in the constellation of Virgo. | |
| Artist's impression of | PSR B1257+12 A planet. |
| Artist's impression of | PSR B1257+12 B. |
| The designation | PSR B1257+12 refers to its coordinates in the B1950 |
| PSR B1257+12 D is a possible extrasolar dwarf plane | |
| It is suspected that a dwarf planet is orbiting | PSR B1257+12 at an average orbital distance of 2.6 |
| predating the 1992 pulsar planets found around | PSR B1257+12 and main-sequence yellow dwarf 51 Pega |
| inclination of the planets orbiting the pulsar | PSR B1257+12 had been determined by measuring their |
| The planets of | PSR B1257+12 are designated from A to D (ordered by |
| An artist's conception of | PSR B1257+12's system of planets |
| net is the innermost object orbiting the pulsar | PSR B1257+12, i.e. a pulsar planet. |
| planets and a possible third around the pulsar | PSR B1257+12. |
| PSR B1257+12A is catalogued as "PSR 1257+12b" on Th | |
| PSR B1257+12A is an extrasolar planet approximately | |
| PSR B1257+12B was the first planet ever discovered | |
| PSR B1257+12B is an extrasolar planet (approximatel | |
| The other two systems are | PSR B1259-63 and LS 5039. |
| Sequence of | PSR B1509-58 images. |
| Size comparison between | PSR B1509-58 and the Crab Nebula. |
| PSR B1509-58 is a pulsar approximately 17,000 light | |
| Tour of | PSR B1509-58. |
| The system is composed of a pulsar ( | PSR B1620-26 A) and a white dwarf (WD B1620-26 or P |
| PSR B1620-26 is a binary star system approximately | |
| arly all extrasolar planets discovered to date, | PSR B1620-26 b was originally detected through the |
| gether with their host stars, it is likely that | PSR B1620-26 b is also about 12.7 billion years old |
| the discovery of a Jupiter-sized planet around | PSR B1620-26, thought to be the oldest known extras |
| The evolution of the | PSR B1620−26 system. |
| At that time, | PSR B1620−26 B was still a main sequence star, with |
| It is theorized that originally | PSR B1620−26 A had another, lower mass white dwarf |
| PSR B1620−26 b was originally detected through the | |
| PSR B1828-10 is a pulsar approximately 11,812 light | |
| PSR B1829-10 (often shortened to PSR 1829-10) is a | |
| Two other pulsars, | PSR B1855+09 and PSR B1937+21 are known to be compa |
| ed to the discovery of the binary pulsar system | PSR B1913+16 by Joseph Taylor and Russell Hulse, fo |
| In the case of | PSR B1913+16, the orbit is inclined at about 45 deg |
| 1974, Hulse and Taylor discovered binary pulsar | PSR B1913+16, which is made up of a pulsar and blac |
| n Bell Burnell, who discovered the first pulsar | PSR B1919+21 in 1967, relates that in the late 1950 |
| er being the discovery of pulsars, specifically | PSR B1919+21, which are rotating neutron stars. |
| He discovered the first millisecond pulsar, | PSR B1937+21, which rotates at a rate far beyond wh |
| m that discovered the first millisecond pulsar, | PSR B1937+21. |
| The | PSR emerged at the end of the 1890s and held its fi |
| P.S.R. Engineering College | |
| ubanovich were instrumental in establishing the | PSR's contacts with Western socialist parties and w |
| PSR has won 5 Golden Quill Awards, presented by The | |
| Rusanov joined the | PSR in 1901, together with such venerable veteran r |
| The activities at | PSR include. |
| "Physicians for Social Responsibility ( | PSR) is the largest physician-led organization in t |
| The focus of | PSR is on patient (or "member," as they are often r |
| PSR J0437-4715 is a pulsar. | |
| ervations indicate that the binary companion of | PSR J0437-4715 is most likely a low-mass helium whi |
| PSR J0437-4715 is the first MSP to have its X-ray e | |
| The pair | PSR J0737-3039 are only some 800,000 km apart, or a |
| itial claim to fame was being the discoverer of | PSR J0737-3039, the first double pulsar (two pulsar |
| PSR J0855-4644, Pulsar. | |
| PSR J1748-2446ad is the fastest-spinning pulsar kno | |
| 42 times per second, and until the discovery of | PSR J1748-2446ad in 2005, it was the fastest-spinni |
| with the second fastest-spinning pulsar known, | PSR J1748-2446ad (which rotates 716 times per secon |
| PSR J1748-2446ad, at 716 Hz, the pulsar with the hi | |
| PSR J1903+0327 appears to require a different forma | |
| PSR J1903+0327 is a millisecond pulsar in a highly | |
| designation was CP 1919 and it is also known as | PSR J1921+2153. |
| PSR J1951+1123 is a pulsar. | |
| PSR J2007+2722 is a 40.8-hertz isolated pulsar in t | |
| and are adopting a psychosocial rehabilitation ( | PSR) model instead. |
| The tactical position adopted by the | PSR represented a compromise between the rural agit |
| ps that left IU: Revolutionary Socialist Party ( | PSR), Revolutionary Communist Party (PCR) and Peruv |
| One of the reasons the school moved to | PSR was that it could partner with established scho |
| ce King from the disaster of 1954, and then his | psr was so high they made him leave. |
| Ideologically and tactically the | PSR was quite diverse, comprising anti-Marxists as |
| involved in the Socialist-Revolutionary Party ( | PSR), which united a variety of populist and revolu |
| me served in the 'Fighting Organisation' of the | PSR, which was responsible for acts of `political t |
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