[HTML][HTML] The external photoevaporation of planet-forming discs
AJ Winter, TJ Haworth - The European Physical Journal Plus, 2022 - Springer
Planet-forming disc evolution is not independent of the star formation and feedback process
in giant molecular clouds. In particular, OB stars emit UV radiation that heats and disperses …
in giant molecular clouds. In particular, OB stars emit UV radiation that heats and disperses …
[HTML][HTML] Outcomes among confirmed cases and a matched comparison group in the Long-COVID in Scotland study
With increasing numbers infected by SARS-CoV-2, understanding long-COVID is essential
to inform health and social care support. A Scottish population cohort of 33,281 laboratory …
to inform health and social care support. A Scottish population cohort of 33,281 laboratory …
Protoplanetary disc truncation mechanisms in stellar clusters: comparing external photoevaporation and tidal encounters
Most stars form and spend their early life in regions of enhanced stellar density. Therefore,
the evolution of protoplanetary discs (PPDs) hosted by such stars are subject to the …
the evolution of protoplanetary discs (PPDs) hosted by such stars are subject to the …
[HTML][HTML] Natural history of long-COVID in a nationwide, population cohort study
Previous studies on the natural history of long-COVID have been few and selective. Without
comparison groups, disease progression cannot be differentiated from symptoms originating …
comparison groups, disease progression cannot be differentiated from symptoms originating …
Stellar clustering shapes the architecture of planetary systems
AJ Winter, JMD Kruijssen, SN Longmore, M Chevance - Nature, 2020 - nature.com
Planet formation is generally described in terms of a system containing the host star and a
protoplanetary disk,–, of which the internal properties (for example, mass and metallicity) …
protoplanetary disk,–, of which the internal properties (for example, mass and metallicity) …
The FRIED grid of mass-loss rates for externally irradiated protoplanetary discs
TJ Haworth, CJ Clarke, W Rahman… - Monthly Notices of …, 2018 - academic.oup.com
We present an open access grid of 3930 calculations of externally evaporating
protoplanetary discs. This spans a range of disc sizes (1–400 au), disc masses, UV field …
protoplanetary discs. This spans a range of disc sizes (1–400 au), disc masses, UV field …
Flybys in protoplanetary discs–II. Observational signatures
N Cuello, F Louvet, D Mentiplay, C Pinte… - Monthly Notices of …, 2020 - academic.oup.com
Tidal encounters in star clusters perturb discs around young protostars. In Cuello et al., we
detailed the dynamical signatures of a stellar flyby in both gas and dust. Flybys produce …
detailed the dynamical signatures of a stellar flyby in both gas and dust. Flybys produce …
[HTML][HTML] True prevalence of long-COVID in a nationwide, population cohort study
Long-COVID prevalence estimates vary widely and should take account of symptoms that
would have occurred anyway. Here we determine the prevalence of symptoms attributable …
would have occurred anyway. Here we determine the prevalence of symptoms attributable …
Prevalent externally driven protoplanetary disc dispersal as a function of the galactic environment
AJ Winter, JMD Kruijssen, M Chevance… - Monthly Notices of …, 2020 - academic.oup.com
The stellar birth environment can significantly shorten protoplanetary disc (PPD) lifetimes
due to the influence of stellar feedback mechanisms. The degree to which these …
due to the influence of stellar feedback mechanisms. The degree to which these …
The influence of the environment on the spin evolution of low-mass stars–I. External photoevaporation of circumstellar discs
Massive stars are strong sources of far-ultraviolet radiation that can be hostile to the
evolution of protoplanetary discs, driving mass-loss by external photoevaporation and …
evolution of protoplanetary discs, driving mass-loss by external photoevaporation and …