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  2. Spiral galaxy - Wikipedia

    en.wikipedia.org/wiki/Spiral_galaxy

    Spiral arms appear visually brighter because they contain both young stars and more massive and luminous stars than the rest of the galaxy. As massive stars evolve far more quickly, [ 27 ] their demise tends to leave a darker background of fainter stars immediately behind the density waves.

  3. Milky Way - Wikipedia

    en.wikipedia.org/wiki/Milky_Way

    In December 2013, astronomers found that the distribution of young stars and star-forming regions matches the four-arm spiral description of the Milky Way. [212] [213] [214] Thus, the Milky Way appears to have two spiral arms as traced by old stars and four spiral arms as traced by gas and young stars. The explanation for this apparent ...

  4. Density wave theory - Wikipedia

    en.wikipedia.org/wiki/Density_wave_theory

    The density wave theory also explains a number of other observations that have been made about spiral galaxies. For example, "the ordering of H I clouds and dust bands on the inner edges of spiral arms, the existence of young, massive stars and H II regions throughout the arms, and an abundance of old, red stars in the remainder of the disk".

  5. Stellar population - Wikipedia

    en.wikipedia.org/wiki/Stellar_population

    Stellar population. Artist's conception of the spiral structure of the Milky Way showing Baade's general population categories. The blue regions in the spiral arms are composed of the younger population I stars, while the yellow stars in the central bulge are the older population II stars. In reality, many population I stars are also found ...

  6. Andromeda Galaxy - Wikipedia

    en.wikipedia.org/wiki/Andromeda_Galaxy

    Neutron stars and black holes can be distinguished mainly by measuring their masses. [110] An observation campaign of NuSTAR space mission identified 40 objects of this kind in the galaxy. [ 111 ] In 2012, a microquasar , a radio burst emanating from a smaller black hole was detected in the Andromeda Galaxy.

  7. Seyfert galaxy - Wikipedia

    en.wikipedia.org/wiki/Seyfert_galaxy

    The Circinus Galaxy, a Type II Seyfert galaxy. Seyfert galaxies are one of the two largest groups of active galaxies, along with quasar host galaxies. They have quasar-like nuclei (very luminous sources of electromagnetic radiation that are outside of our own galaxy) with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, [1] but unlike quasars, their ...

  8. Young adults are getting cold feet about their highly ...

    www.aol.com/finance/young-adults-getting-cold...

    Young adults’ anxiety regarding an incoming inheritance has been also covered by a 2024 report from New York Life. The insurance company found that only 42% of the 15% of adults that expected an ...

  9. Elliptical galaxy - Wikipedia

    en.wikipedia.org/wiki/Elliptical_galaxy

    Elliptical (E) galaxies are, together with lenticular galaxies (S0) with their large-scale disks, and ES galaxies [ 2][ 3][ 4] with their intermediate scale disks, a subset of the "early-type" galaxy population. Most elliptical galaxies are composed of older, low-mass stars, with a sparse interstellar medium, and they tend to be surrounded by ...