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A search for millisecond radio bursts from Messier 82
S Paine, T Hawkins, D R Lorimer, J Stanley, J Kania, F Crawford and N Fairfield Monthly Notices of the Royal Astronomical Society 528(4) 6340 (2024) https://doi.org/10.1093/mnras/stae344
Hierarchical Bayesian approach for estimating physical properties in nearby galaxies: Age Maps (Paper II)
M Carmen Sánchez-Gil, Emilio J Alfaro, Miguel Cerviño, et al. Monthly Notices of the Royal Astronomical Society 483(2) 2641 (2019) https://doi.org/10.1093/mnras/sty3106
Deciphering an evolutionary sequence of merger stages in infrared-luminous starburst galaxies atz∼ 0.7
Young star clusters in circumnuclear starburst rings
Richard de Grijs, Chao Ma, Siyao Jia, Luis C. Ho and Peter Anders Monthly Notices of the Royal Astronomical Society 465(3) 2820 (2017) https://doi.org/10.1093/mnras/stw2806
STARBURST-DRIVEN GALACTIC SUPERBUBBLES RADIATING TO 10 K
The VMC survey – XVI. Spatial variation of the cluster formation activity in the innermost regions of the Large Magellanic Cloud
Andrés E. Piatti, Richard de Grijs, Vincenzo Ripepi, et al. Monthly Notices of the Royal Astronomical Society 454(1) 839 (2015) https://doi.org/10.1093/mnras/stv2054
STAR CLUSTER DISRUPTION IN THE STARBURST GALAXY MESSIER 82
Evolution of M82-like starburst winds revisited: 3D radiative cooling hydrodynamical simulations
C. Melioli, E. M. de Gouveia Dal Pino and F. G. Geraissate Monthly Notices of the Royal Astronomical Society 430(4) 3235 (2013) https://doi.org/10.1093/mnras/stt126
The NGC 5253 star cluster system – I. Standard modelling and infrared-excess sources
Richard de Grijs, Peter Anders, Erik Zackrisson and Göran Östlin Monthly Notices of the Royal Astronomical Society 431(3) 2917 (2013) https://doi.org/10.1093/mnras/stt392
The stochastic nature of stellar population modelling
No compelling evidence of significant early star cluster disruption in the Large Magellanic Cloud
Richard de Grijs, Simon P. Goodwin and Peter Anders Monthly Notices of the Royal Astronomical Society 436(1) 136 (2013) https://doi.org/10.1093/mnras/stt1541
AGE AND MASS CONSTRAINTS FOR A YOUNG MASSIVE CLUSTER IN M31 BASED ON SPECTRAL ENERGY DISTRIBUTION FITTING