It is mainly in supernova explosions that part of the matter of the star - NOT all of it - goes back into space; as a result, some of it eventually ends up in new solar systems, such as our Solar System.
The result of this is that our Solar System has some heavy elements, which were not present when the Universe began.
Please note that this "recycling" can't go on forever. Part of the mass stays in the star remainders; a supernova may collapse into a neutron star or a black hole. Also, the matter that goes out into space has more heavy elements than the original mass of the star that went supernova. In other words, it contains less hydrogen, which is used as fuel for stars.
extinction
by observing in high-energy wavelengths such as X rays and long wavelengths of light such as radio waves
The interstellar medium is enriched with heavy elements by the remnants of supernovas. A supernova is the spectacular explosion at the end of a stars life when it collapses in on itself.
red light from the emission nebula
The interstellar medium is an extremely sparse (tenuous) mix of gas and dust, some of the gas being ionized, some atomic, and some molecular. By composition the gas is largely hydrogen, with smaller amounts of helium and very small amounts of heavier elements. There are also cosmic rays which are protons and nuclei which have been accelerated to near-relativistic speeds. In cooler, high-density areas, the interstellar medium can become as dense as one ten-billionth that of air.
Brian M. Cancellieri has written: 'Interstellar medium' -- subject(s): Interstellar matter
extinction
Visible light against electrons combined with ionized hydrogen create the "reddening" effect in the Interstellar Medium.
Ginevra Trinchieri has written: 'The environmental impact of intra-cluster medium on the interstellar medium in early type galaxies' -- subject(s): X ray astronomy, Galaxies, Interstellar matter
W. B. Burton has written: 'The galactic interstellar medium' -- subject(s): Astrophysics, Interstellar matter, Molecular clouds
Although solid, gas and liquid are the most common states of matter on Earth, much of the baryonic matter of universe is in the form of hot Plasma, both as rarefied interstellar medium and as dense stars.
A galaxy is a vast number of stars together with the interstellar medium and dark matter bound together by gravity.
Gravity plays an important role in the birth of a star. It concentrates matter in the interstellar medium to the point where fusion occurs.
Gravity plays an important role in the birth of a star. It concentrates matter in the interstellar medium to the point where fusion occurs.
Of the visible, baryonic matter in the universe, about 0.1% is not plasma, according to some hurried estimates. This includes the large gas giants, such as Saturn and Jupiter. Most all of the Sun's hydrogen and helium is ionized, and most of the interstellar medium as well.However, ordinary matter, the stuff plasma is made up of, only constitutes about 5% of the total mass-energy of the universe. Some 27% is dark matter, and it is not known whether dark matter can form plasma of any kind. It's safe to say that less than 5% of the total mass-energy of the universe comes as baryonic plasma.
Hydrogen
"A compressible medium." "A displaceable medium."