no code implementations • 11 Feb 2021 • Zeinab Khorrami, Maud Langlois, Paul C. Clark, Farrokh Vakili, Anne S. M. Buckner, Marta Gonzalez, Paul Crowther, Richard Wunsch, Jan Palous, Stuart Lumsden, Estelle Moraux
Our aim was to (i) increase the number of resolved sources in the core of R136, and (ii) to compare with the first epoch to classify the properties of the detected common sources between the two epochs.
Solar and Stellar Astrophysics Astrophysics of Galaxies
