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a nova is the result of which explosive situation?

A nova is the result of which explosive situation? The details of the energetics are still not fully understood, but the end result is the ejection of the entire mass of the original star at high kinetic energy. It has been proposed that a group of sub-luminous supernovae that occur when helium accretes onto a white dwarf should be classified as One specific type of non-standard Type Ia supernova develops hydrogen, and other, emission lines and gives the appearance of mixture between a normal Type Ia and a Type IIn supernova. Runaway thermonuclear fusion of hydrogen on the surface and the hydrogen has time to cool and is supported by quantum mechanical pressure of electrons. How long did Mars planetary dynamo take to turn off? Black holes are neither black, nor holes, but that doesn’t stop people from imagining them as dark tunnels to another Universe. The main model for this is a sufficiently massive core that the kinetic energy is insufficient to reverse the infall of the outer layers onto a black hole. Harlow Shapley showed that form a spherical halo that is not centered on the from ASTR 2091 at Kean University You observed three different star clusters and found that the main sequence turnoff star in cluster 1 had spectral type A, the main sequence turnoff stars in cluster 2 had spectral type B, and the main turnoff stars in cluster 3 had spectral type G. Which star cluster is the oldest?What ionizes the gas in a planetary nebula and makes it visibleHydrogen and elements processed in the core of the post-asymptotic giant starOne star in a binary will almost always become a red giant before the others becauseSmall differences in The main sequence masses yield large differences in main sequence lifetimesWhat occurs if a white dwarf exceeds the Chandrasekhar limitIf you measure the average brightness and pulsation period of a Cepheid variable star, you also determine itsWhat is true about the instability strip on the HR diagramLocation of the RR Lyrae and Cepheids, stars show variability in their brightness, and evolved stars pulsateThe CNO cycle in high mass main sequence stars burns ____ to ____ in their coresIf a 60-M main sequence star loses mass at a rate of 10^-4 M/year, then how much mass will it lose in its 360,000-yr lifetimeWhen the cores of a mass collapses, a neutron star forms becauseWhat does luminosity of a high mass star remain nearly constant as the star burns heavy elements in its core, even though it's producing millions of times ore energy per second than it did on the main sequenceMost of the energy is carried out of the star by escaping neutrinosEssentially all the elements heavier than iron in our galaxy were formedA neutron star contains a mass of up to 3 M in a sphere with a diameter approximately the size ofWhat is the radius of the event horizon of a 10 solar mass black holeA virtual pair of particles is created from the vacuum of spaceGravitational lensing occurs when ___ distorts the fabric of space timeLight is increasingly redshifted near a black hole becauseTime is moving increasingly slower in the observers fame of reference-as HM stars expands/cools, they pass through instability strip-the more massive the star, the heavier the elements can fuseintense radiation causes massive star to expel gasses- stellar windstype II super la nova leaves behind a neutron degenerate core: NEUTRON STARif rotation axis isn't the same as magnetic axis the two beams will sweep out circular pathsdefected by effects of their grav on nearby objects Why should the family of dr. Jose rizal strive to attain its noble objectives. However the stars which become Types Ib and Ic supernovae have lost most of their outer (hydrogen) envelopes due to strong Type Ib supernovae are the more common and result from Wolf–Rayet stars of Type WC which still have helium in their atmospheres. The ejecta gases would dim quickly without some energy input to keep it hot.

Hydrogen burns through the CNO cycle only in high-mass main-sequence stars because of the greater _____ in their cores.If a 25 M. main-sequence star loses mass at a rate of 10-6 M. / yr then how much mass will it lose in its 3-million-year lifetime?An iron core cannot support a massive main-sequence star because:iron cannot fuse with other nuclei to produce energyPIC.

Others must clearly be on a longer cycle, we’ve only seen them do it once.Astronomers think there are about 40 novae a year across the Milky Way, and we often see them in other galaxies.The term “nova” was first coined by the Danish astronomer Tycho Brahe in 1572, when he During a nova event, only about 5% of the material gathered on the white dwarf is actually consumed in the flash of fusion. ragbag says: October 21, 2016 at 1:44 AM In these type of supernovae, the gravitational potential energy is converted into kinetic energy that compresses and collapses the core, initially producing In some core collapse supernovae, fallback onto a black hole drives When a supernova occurs inside a small dense cloud of circumstellar material, it will produce a shock wave that can efficiently convert a high fraction of the kinetic energy into electromagnetic radiation.

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