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RELATION BETWEEN TIDAL DISRUPTION EVENTS AND HOST GALAXIES

Image: Artistic illustration of a black hole divouring a star. Credit: NASA/Goddard Space Flight Center/CI Lab
 
A tidal disruption event occurs when a star gets close enough to a supermassive black hole's event horizon and is pulled apart by the black hole's tidal forces.
In a recent paper (French, Arcavi & Zabludoff, 2016 ApJL) the authors show that the tidal disruption events occur more frequently in host galaxies with strong Balmer line absorption. This feature indicates low levels of current star formation.





The Balmer lines in atomic physics, is the designation of one of a set of six named series describing the spectral line emissions of the hydrogen atom. The Balmer series is characterized by the electron transitioning from n > 2 to n = 2, where n refers to the radial quantum number or principal quantum number of the electron.

In the simplified Rutherford Bohr model of the hydrogen atom, the Balmer lines result from an electron jump between the second energy level closest to the nucleus, and those levels more distant. Shown here is a photon emission. (https://en.wikipedia.org/wiki/Balmer_series)





The connection tidal-disruption/host-galaxy may be due to the fact that these host galaxies have had a recent galaxy-galaxy merger. Such event increases the possibility of formation of black-hole binaries, perturbed stellar orbits and a spatially-concentrated population of A giant stars.


Figure: Tidal disruption of a star. Credit: NASA/Goddard Space Flight Center/Swift


▪ French, Arcavi & Zabludoff (ApJL) - Tidal drisuption events prefer unusual host galaxies. (arXiv)


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