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Mysterious Stars Surround Andromeda's Black Hole

UltimaGuy writes to tell us that Yahoo is running a story about a recent discovery that shows the source of strange blue light coming from the center of the Andromeda galaxy. The light is actually a cluster of stars circling the galaxy's central black hole with immense orbital velocity. From the article: "Such frenetic activity was thought to prevent star formation. Stars form when a knot of gas and dust collapses under its own gravity."

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  1. Elements past iron by benhocking · · Score: 4, Informative

    Elements past iron can only be created in a supernova explosion. Google on "supernova elements" for more information. Of course, the element synthesis during a supernova explosion is due to fusion, but I'm not sure one could call it "star fusion".

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    1. Re:Elements past iron by MaskedSlacker · · Score: 5, Informative

      Actually its neutron accretion that produces elements heavier than iron, not fusion. Iron disintegrates at temperatures lower than what it will fuse at.

    2. Re:Elements past iron by MaskedSlacker · · Score: 5, Informative

      No, because hydrogen is a single proton, not a single neutron. I forget the exact mechanics of neutron accretion, as its not my field of direct study, but it occurs in two forms, the r-process (rapid) and the s-process(slow) (we physicists are not known for being creative with names). The r-process occurs in supernovae when heavy nuclei are bombarded by many neutrons, ad rather than splitting the target nuclei, the neutrons stick (at the same time the nuclei are radiating particles away, but not as fast as they are gaining them). Once the process stops, the new, super neutron rich nuclei give off beta radiation (changing neturons into protons) until they reach a stable configuration. The s-process occurs in large, but otherwise stable stars. This process however only produces elements as heavy as lead. Anything heavier is produced by the r-process.

  2. An escaping star?? HA! by lightyear4 · · Score: 4, Informative

    Wouldnt matter too much...our Milky Way and Andromeda are on a slow collision course anyway - by the time an ejected star got here, the rest of the galaxy would be right behind it. But no need to go hide in a cave just yet, we've still got about 3 billion years.

  3. Re:Well... by swelke · · Score: 5, Informative

    That's quite possible. If they formed in a wider orbit around the black hole, for example, they could well have been caught by tidal drag and slowly moved into lower orbits.

    The real question is how they can exist at all in such a low orbit (or, more accurately, how they can exist in such a strong gravity gradient). What happens is that if they tidal difference between the two sides of the star (the difference between the black hole's gravity at the closest edge of the star and that on the furthest edge) exceeds the star's escape velocity, matter will be able to leave the star and it just falls apart. The implication (which the Yahoo! article was too low-tech to get right) was that the stars must be very dense. A dense star will have both (a) less distance between that nearest and furthest edge and (b) a steeper gravity well for material to get out of in the first place.

    The other interesting bit is the rather close estimate of the black hole's mass. Most of the other estimates of galactic center black hole masses I've seen are based on things orbiting them far more distantly, such as 10-100 light years.

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