2017 - Member of the Royal Irish Academy
Astrophysics, Stars, Astronomy, Metallicity and Wolf–Rayet star are his primary areas of study. His works in Stellar evolution, Galaxy, Supergiant, Star cluster and Star formation are all subjects of inquiry into Astrophysics. Paul A. Crowther interconnects Line and Star in the investigation of issues within Stellar evolution.
Stars is often connected to Spectral line in his work. The Metallicity study combines topics in areas such as Supernova and Bright giant. Paul A. Crowther usually deals with Wolf–Rayet star and limits it to topics linked to Emission spectrum and Envelope.
The scientist’s investigation covers issues in Astrophysics, Stars, Astronomy, Wolf–Rayet star and Galaxy. His Astrophysics research is multidisciplinary, relying on both Spectroscopy and Spectral line. He combines topics linked to Line with his work on Stars.
His work is connected to K-type main-sequence star, Milky Way, Nebula, Stellar mass loss and Star, as a part of Astronomy. His Wolf–Rayet star research incorporates themes from Emission spectrum and Spiral galaxy. His research ties Supernova and Galaxy together.
Paul A. Crowther mostly deals with Astrophysics, Stars, Large Magellanic Cloud, Astronomy and Galaxy. His work on Spectral line expands to the thematically related Astrophysics. As a part of the same scientific study, he usually deals with the Spectral line, concentrating on Spectroscopy and frequently concerns with Stellar population.
His study in Nebula, Supergiant, Star cluster, Stellar classification and Effective temperature is done as part of Stars. His research integrates issues of Main sequence, Star formation, Stellar mass, Initial mass function and Orbital period in his study of Large Magellanic Cloud. The study incorporates disciplines such as Metallicity and O-type star in addition to Stellar evolution.
Paul A. Crowther spends much of his time researching Astrophysics, Stars, Large Magellanic Cloud, Galaxy and Nebula. He focuses mostly in the field of Astrophysics, narrowing it down to matters related to Spectral line and, in some cases, Envelope. His Large Magellanic Cloud research includes elements of Star cluster and Stellar mass.
His Galaxy research is classified as research in Astronomy. Paul A. Crowther has included themes like Astronomical spectroscopy, Interstellar medium and Balmer series in his Nebula study. His study explores the link between Metallicity and topics such as Stellar classification that cross with problems in Emission spectrum and Critical mass.
This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.
Physical Properties of Wolf-Rayet Stars
Paul A. Crowther.
Annual Review of Astronomy and Astrophysics (2007)
The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 Msun stellar mass limit
Paul A Crowther;Olivier Schnurr;Raphael Hirschi;Norhasliza Yusof.
arXiv: Solar and Stellar Astrophysics (2010)
Realistic ionizing fluxes for young stellar populations from 0.05 to 2 Z
Linda J. Smith;Richard P. F. Norris;Paul A. Crowther.
Monthly Notices of the Royal Astronomical Society (2002)
Realistic Ionizing Fluxes for Young Stellar Populations from 0.05 to twice solar metallicity
Linda J. Smith;Richard P. F. Norris;Paul A. Crowther.
arXiv: Astrophysics (2002)
The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 M⊙ stellar mass limit
Paul A. Crowther;Olivier Schnurr;Raphael Hirschi;Raphael Hirschi;Norhasliza Yusof.
Monthly Notices of the Royal Astronomical Society (2010)
The VLT-FLAMES Tarantula Survey I: Introduction and observational overview
C. J. Evans;W. D. Taylor;V. Henault-Brunet;H. Sana.
arXiv: Solar and Stellar Astrophysics (2011)
The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population
H. Sana;A. de Koter;A. de Koter;S.E. de Mink;S.E. de Mink;P.R. Dunstall.
Astronomy and Astrophysics (2013)
A Neutron Star with a Massive Progenitor in Westerlund 1
M. P. Muno;J. S. Clark;P. A. Crowther;S. M. Dougherty.
arXiv: Astrophysics (2005)
Physical parameters and wind properties of galactic early B supergiants
P. A. Crowther;D. J. Lennon;N. R. Walborn.
Astronomy and Astrophysics (2006)
The empirical metallicity dependence of the mass-loss rate of O- and early B-type stars
M.R. Mokiem;A. De Koter;J.S. Vink;J. Puls.
Astronomy and Astrophysics (2007)
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