beta decay of heavy isotopes of indium.
question: how do these stars form?, context: Tin is generated via the long S-process in low-to-medium mass stars (with masses of 0.6 to 10 times that of Sun). It arises via beta decay of heavy isotopes of indium.
how do these stars form?
It arises via beta decay of heavy isotopes of indium.
Tin is generated via the long S-process in low-to-medium mass stars (with masses of 0.6 to 10 times that of Sun). It arises via beta decay of heavy isotopes of indium.
It arises via <hl> beta decay of heavy isotopes of indium. <hl>
Tin is generated via the long S-process in low-to-medium mass stars (with masses of 0.6 to 10 times that of Sun). It arises via <hl> beta decay of heavy isotopes of indium. <hl>
Tin is generated via the long S-process in low-to-medium mass stars (with masses of 0.6 to 10 times that of Sun). <hl> It arises via beta decay of heavy isotopes of indium. <hl>