KITP: blue straggler stars

Blue straggler stars are, formally, main sequence stars that are too blue and bright on the colour-magnitude diagram - they are more massive than they ought to be given their age, is the other way of looking at it.
They are found in the field, and you might rightly ponder how we can tell, but in globular clusters there are lots, they really stick out, and they are rather fascinating.
And they make great Hubble Space Telescope targets, being rather blue, in crowded regions and teach you about physics, stellar processes etc.

Blue Straggler Stars (wiki):



Nice illustration of Blue Stragglers on the Colour-Magnitude diagram in M55, from Jerjen at ANU

So there are essentially two ways to make blue stragglers:
you can "decant" a star onto a companion in a close orbit, as suggested by McCrea many years ago - this basically requires a close binary which will evolve into contact - the details are messy, but this can "clearly" happen at some level and provides a background rate for stellar rejuvenation;
or, you can have two (or more) stars go "splat" - hydrodynamic collisions between stars, either mildly hyperbolic collision during direct encounters in very dense clusters, or sup-hyperbolic collisions during binary encounters in moderate or dense clusters.

Famously, the physics of the latter process are simpler - it is rapid, and the shocks are mild, so the collision is near isentropic and the merged stellar product is essentially layered mix of the original stars, but local specific entropy.
Specific entropy within a star is generally higher in the center and lower on the outside.
On the main sequence the mean specific entropy is a monotonic function of mass, but as stars evolve onto the giant branch the mean specific entropy becomes lower.
So we mostly think we understand the structure of stars after hyperbolic hydrodynamic collisions, and their subsequent evolution, modulo rotation and magnetic fields etc.



click to embiggen

Associated press release

The decanting process, not so simple...



yup, clusters really are crowded



'course there are other blue things

Tags

More like this

whee, we make stars go splat again! what exactly does happen when stars collide, just ordinary low mass main sequence stars Glebbeek and Pols A&A 2008 - v 488 p 1007 and p 1017 BSE: binary stellar evolution code - Hurley et al 2002 from Tout et al 1997 - mass is wrong, - lifetime is wrong…
we continue contemplation of stars going splat there are blue stragglers in dwarf galaxies they are presumably binaries merged through McCrea type I mass transfer we're not sure exactly how that works in detail, but it must happen because we see it in progress - ie we see contact binaries on the…
it is still raining?! so we have an east coaster telling us about actual data on x-ray binaries in clusters, globular clusters in other galaxies... there is an open-to-the-program-members blog over on the cluster09 wikispace. It has some good summary of yesterdays in depth discussion on runaway…
it is raining, might as well liveblog the morning session... runaway mergers of colliding stars - the quick and dirty intro... stars are, in fact extended bodies. This is mostly irrelevant to astronomers, since typical stellar separations are very large. But, in dense stellar clusters, the…