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when the core of a massive star collapses, a neutron star forms because

When the progenitor star is below about 20 M ☉ – depending on the strength of the explosion and the amount of material that falls back – the degenerate remnant of a core collapse is a neutron star. a. Protons and electrons combine to minimize electromagnetic forces. b. This blue light indicates that these regions contain:Every pulsar is a neutron star, but not every neutron star is a pulsar.The Type II supernova that created the Crab Nebula was seen by Chinese and Arab astronomers in the year 1054 CE. When a star goes supernova, the core of … Please deactivate your ad blocker in order to see our subscription offerWith the highest density of any known space object, neutron stars can beam radiation across the galaxy. For example, do the incredible pressures found within neutron stars break neutrons down into soups of still tinier subatomic particles known as "These stars are very exotic," study co-author Maura McLaughlin at West Virginia University in Morgantown The newly measured neutron star, called J0740+6620, lies about 4,600 light-years from Earth.

New York, the path of light is longer. These light curves have an average decay rate of 0.008 The difference in the shape of the light curves is believed to be caused, in the case of Type II-L supernovae, by the expulsion of most of the hydrogen envelope of the progenitor star.The "n" denotes narrow, which indicates the presence of narrow or intermediate width hydrogen emission lines in the spectra. Any star that burns silicon to iron will collapse when the iron core passes the Chandrasekhar limit. what is the single most important determinant of the qualitiesas the hydrogen atoms at the core are consumed (fusion)?star burning hydrogen into helium into a shell around the corehow long ago parent star died nebulous radius & expansion velocitymain sequence, red giant, planetary nebula, white dwarfwhat happens to the rotational rate of a massive star that has undergone a type II supernova and become a neutron star?hydrogen and elements processed in the core of the PAGB starone star in a binary will always become a red giant before the other becausesmall differences in main sequence masses yield large differences in main sequence massesyou can determine a stars distance if you measure what?the average brightness and pulsation period of a Cepheid variable starthe CNO cycle in high mass main sequence burns whatwhen the core of a massive star collapses, a neutron star forms becausemost energy is carried out of the star by escaping neutrinosessentially all the elements heavier than iron in our galaxy were formed by what?hawking radiation is emitted by a black hole when a virtual pair of particles is created from?any massive object distorts the fabric of space timelight is increasingly redshifted near a black hole becausetime is moving increasingly slower in the observers frame of reference When the core of a massive star collapses, a neutron star forms because: a. all the charged particles are ejected in the resulting explosion. High-mass stars differ from low-mass stars in that they burn helium to carbon when on the main sequence.The main difference between Cepheid stars and RR Lyrae stars is:If you measure the average brightness and pulsation period of a Cepheid variable star, you can also determine its:run out of nuclear fuel in their core, and the cores collapseFusion reactions that create chemical elements heavier than oxygen require energy input; thus, these reactions cannot provide a star with power.Cepheid variable stars are important because we can use them to determine the distance to any stellar group that contains some of these stars.In the CNO cycle, carbon is used a catalyst for the fusion of hydrogen to helium. When the core of a massive star collapses, a neutron star forms because: protons and electrons combine to make neutrons The collapse of the core of a high-mass star at the end of its life lasts approximately:

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