5 definitions found From The Collaborative International Dictionary of English v.0.48 [gcide]: Nova \No"va\ (n[=o]"v[.a]), n.; pl. L. {Novae} (n[=o]"v[=e]), E. {Novas} (n[=o]"v[.a]z). [L., fem. sing. of novus new.] (Astron.) A star which suddenly increases in brightness thousands of times, then fades back to near its original intensity. It may appear as a "new" star if its original brightness was too low for routine observation. A star which suddenly increases in brightness to many millions of times its original intensity is a {supernova}, and the postulated mechanisms for the increases of brightness of novae and supernovae are different. Note: The most important modern novae are: {No"va Co*ro"nae Bo`re*a"lis}[1866]; {No"va Cyg"ni}[1876]; {No"va An*dro"me*dae}[1885]; {No"va Au*ri"gae}[1891-92]; {No"va Per"se*i}[1901]. There are two novae called {Nova Persei}. They are: (a) A small nova which appeared in 1881. (b) An extraordinary nova which appeared in Perseus in 1901. It was first sighted on February 22, and for one night (February 23) was the brightest star in the sky. By July it had almost disappeared, after which faint surrounding nebulous masses were discovered, apparently moving radially outward from the star at incredible velocity. [Webster 1913 Suppl. +PJC] From WordNet (r) 2.0 [wn]: nova n : a star that ejects some of its material in the form of a cloud and become more luminous in the process [also: {novae} (pl)] From Moby Thesaurus II by Grady Ward, 1.0 [moby-thes]: 40 Moby Thesaurus words for "nova": Beehive, Cepheid variable, Hertzsprung-Russell diagram, Hyades, Messier catalog, NGC, Pleiades, Seven Sisters, absolute magnitude, binary star, black hole, double star, dwarf star, fixed star, giant star, globular cluster, gravity star, magnitude, main sequence star, mass-luminosity law, neutron star, open cluster, populations, pulsar, quasar, quasi-stellar radio source, radio star, red giant star, relative magnitude, sky atlas, spectrum-luminosity diagram, star, star catalog, star chart, star cloud, star cluster, stellar magnitude, supernova, variable star, white dwarf star From The Free On-line Dictionary of Computing (27 SEP 03) [foldoc]: NovaA {minicomputer}(?), introduced some time before 1978, with four 16-bit {accumulator}s, AC0 to AC3 and a 15 bit {program counter}. A later model also had a 15-bit {stack pointer} and {frame pointer}. AC2 and AC3 could be used for indexed addresses and AC3 was used to store the return address on a {subroutine} call. Apart from the small {register set}, the NOVA was an ordinary {CPU} design. Memory could be access indirectly through addresses stored in other memory locations. If locations 0 to 3 were used for this purpose, they were auto-incremented after being used. If locations 4 to 7 were used, they were auto-decremented. Memory could be addressed in 16-bit words up to a maximum of 32K words (64K bytes). The instruction cycle time was 500 {nanoseconds}(?) cycle time for each. The Nova originally used {core memory} though later on they gained {dynamic RAM}. Like the {PDP-8}, the {Data General} Nova was also copied, not just in one, but two implementations - the {Data General MN601} and {Fairchild 9440}. Luckily, the NOVA was a more mature design than the PDP-8. Another CPU, the {PACE}, was based on the NOVA design, but featured 16-bit addresses (instead of the Nova's 15), more {addressing mode}s and a 10-level {stack} (like the {Intel 8008}). [Date, speed, mini?] (1996-03-01) From U.S. Gazetteer (1990) [gazetteer]: Nova, OH Zip code(s): 44859
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