no code implementations • 8 Oct 2020 • Jeremy Lim, Emily Wong, Youichi Ohyama, Tom Broadhurst, Elinor Medezinski
The sustained formation of these star clusters demonstrates that progenitor GCs can form over cosmic history from cooled intracluster gas, thus contributing to both the large number and broad colour dispersion$-$owing to an age spread, in addition to a spread in metallicity$-$of GCs in massive elliptical galaxies.
Astrophysics of Galaxies
no code implementations • 3 Apr 2020 • Gerrit Schellenberger, Laurence P. David, Jan Vrtilek, Ewan O'Sullivan, Jeremy Lim, William Forman, Ming Sun, Francoise Combes, Philippe Salome, Christine Jones, Simona Giacintucci, Alastair Edge, Fabio Gastaldello, Pasquale Temi, Fabrizio Brighenti, Sandro Bardelli
This indicates that the two giant molecular clouds seen in absorption are most likely within the sphere of influence of the supermassive black hole.
Astrophysics of Galaxies
