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19952024
most citedBinary Population and Spectral Synthesis Version 2.1: construction, observational verification and new results

953 citations · 10.8k across the 245 of their papers we have counts for

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Showing 2017Show all

8 papers · 1 filter

physics.app-ph2017

Bright polariton OLEDs operating in the ultra-strong coupling regime

Armando Genco, Alessandro Ridolfo, Salvatore Savasta +3

The generation and control of exotic phenomena in organic electroluminescent microcavities, such as polariton lasing and non-linear optical effects, operating in strong and ultra-s…

astro-ph.SR2017953 cited

Binary Population and Spectral Synthesis Version 2.1: construction, observational verification and new results

J. J. Eldridge, E. R. Stanway, L. Xiao +6

The Binary Population and Spectral Synthesis (BPASS) suite of binary stellar evolution models and synthetic stellar populations provides a framework for the physically motivated an…

astro-ph.EP201763 cited

CO emission tracing a warp or radial flow within 100 au in the HD 100546 protoplanetary disk

Catherine Walsh, Cail Daley, Stefano Facchini +1

We present spatially resolved ALMA images of CO J=3-2 emission from the protoplanetary disk around HD100546. We model the spatially-resolved kinematic structure of the CO emission.…

astro-ph.GA201732 cited

Galaxy And Mass Assembly (GAMA): The Consistency of GAMA and WISE Derived Mass-to-Light Ratios

T. Kettlety, J. Hesling, S. Phillipps +11

Recent work has suggested that mid-IR wavelengths are optimal for estimating the mass-to-light ratios of stellar populations and hence the stellar masses of galaxies. We compare st…

astro-ph.GA201745 cited

The Magellanic Inter-Cloud Project (MAGIC) III: First spectroscopic evidence of a dwarf stripping a dwarf

Ricardo Carrera, Blair C. Conn, Noelia E. D. Noël +2

The Magellanic Bridge (MB) is a gaseous stream that links the Large (LMC) and Small (SMC) Magellanic Clouds. Current simulations suggest that the MB forms from a recent interaction…

astro-ph.GA201722 cited

How do binary clusters form?

Becky Arnold, Simon P. Goodwin, Daniel W. Griffiths +1

Approximately 10 per cent of star clusters are found in pairs, known as binary clusters. We propose a mechanism for binary cluster formation; we use N-body simulations to show that…