pyx$65912$ - definição. O que é pyx$65912$. Significado, conceito
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O que (quem) é pyx$65912$ - definição

RECURRENT NOVA STAR
T pyx; T Pyx
  • AAVSO]] [[light curve]] of [[recurrent nova]] T Pyx from April 13 to May 6, 2011. Up is brighter and down is fainter.
  • bandpasses]].
  • The location of T Pyxidis (circled in red).

pyx         
WIKIMEDIA DISAMBIGUATION PAGE
PYX
[p?ks]
(also pix)
¦ noun
1. Christian Church the container in which the consecrated bread of the Eucharist is kept.
2. (in the UK) a box at the Royal Mint in which specimen gold and silver coins are deposited to be tested annually.
Origin
ME: from L. pyxis, from Gk puxis 'box'.
Pyx         
WIKIMEDIA DISAMBIGUATION PAGE
PYX
·noun ·same·as Pyxis.
II. Pyx ·noun The box in which the compass is suspended; the binnacle.
III. Pyx ·noun The box, case, vase, or tabernacle, in which the host is reserved.
IV. Pyx ·vt To test as to weight and fineness, as the coins deposited in the pyx.
V. Pyx ·noun A box used in the British mint as a place of deposit for certain sample coins taken for a trial of the weight and fineness of metal before it is sent from the mint.
pyx         
WIKIMEDIA DISAMBIGUATION PAGE
PYX
n.
Box (especially that in which the host is kept), tabernacle, vessel, pyxis.

Wikipédia

T Pyxidis

T Pyxidis (T Pyx) is a recurrent nova and nova remnant in the constellation Pyxis. It is a binary star system and its distance is estimated at about 4,783 parsecs (15,600 light-years) from Earth. It contains a Sun-like star and a white dwarf. Because of their close proximity and the larger mass of the white dwarf, the latter draws matter from the larger, less massive star. The influx of matter on the white dwarf's surface causes periodic thermonuclear explosions to occur.

The usual apparent magnitude of this star system is 15.5, but there have been observed eruptions with maximal apparent magnitude of about 7.0 in the years 1890, 1902, 1920, 1944, 1966 and 2011. Evidence seems to indicate that T Pyxidis may have increased in mass despite the nova eruptions, and is now close to the Chandrasekhar limit when it might explode as a supernova. When a white dwarf reaches this limit it will collapse under its own weight and cause a type Ia supernova.