D. J. Lennon mainly investigates Astrophysics, Astronomy, Stars, Galaxy and Metallicity. Supergiant, Stellar evolution, O-type star, Stellar classification and Large Magellanic Cloud are subfields of Astrophysics in which his conducts study. The various areas that D. J. Lennon examines in his Stellar evolution study include Photosphere, Stellar mass and Main sequence.
His study explores the link between Large Magellanic Cloud and topics such as Young stellar object that cross with problems in Photometry, Nebula, Spectral energy distribution and Stellar atmosphere. His Stars research is multidisciplinary, relying on both Spectral line and Luminosity. The study incorporates disciplines such as Small Magellanic Cloud and Bright giant in addition to Metallicity.
His scientific interests lie mostly in Astrophysics, Stars, Astronomy, Supergiant and Galaxy. Astrophysics is often connected to Spectral line in his work. D. J. Lennon combines topics linked to Luminosity with his work on Stars.
His research in Supergiant intersects with topics in Line, Atmosphere and Luminous blue variable. The Stellar evolution study combines topics in areas such as Main sequence and Stellar atmosphere. D. J. Lennon combines subjects such as Initial mass function and Nebula with his study of Large Magellanic Cloud.
His primary areas of investigation include Astrophysics, Stars, Large Magellanic Cloud, Stellar evolution and Metallicity. His research in O-type star, Red supergiant, Star, Radial velocity and Star formation are components of Astrophysics. His Stars study integrates concerns from other disciplines, such as Spectral line and Galaxy.
His work on Stellar classification and Supergiant as part of general Spectral line research is frequently linked to Mixing, bridging the gap between disciplines. D. J. Lennon interconnects Milky Way, Luminosity, OB star, Star cluster and Stellar mass in the investigation of issues within Large Magellanic Cloud. His research investigates the connection between Metallicity and topics such as Main sequence that intersect with problems in Stellar atmosphere, Surface gravity, Stellar black hole and Effective temperature.
D. J. Lennon focuses on Astrophysics, Stars, Large Magellanic Cloud, Star cluster and Stellar evolution. His is doing research in Star formation, O-type star, Astrometry, Nebula and Supergiant, both of which are found in Astrophysics. The concepts of his Supergiant study are interwoven with issues in Spectroscopy, Supernova, Stellar population, SIMBAD and Photometry.
His work deals with themes such as Spectral line and Galaxy, which intersect with Stars. He has researched Large Magellanic Cloud in several fields, including OB star, Stellar mass and Radial velocity. His Local Group research is classified as research in Astronomy.
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O-star mass-loss and wind momentum rates in the Galaxy and the Magellanic Clouds Observations and theoretical predictions
J. Puls;R. P. Kudritzki;A. Herrero;A. W. A. Pauldrach.
Astronomy and Astrophysics (1996)
The INT Photometric Hα Survey of the Northern Galactic Plane (IPHAS)
Janet E. Drew;Robert Greimel;Mike J. Irwin;Amornrat Aungwerojwit.
Monthly Notices of the Royal Astronomical Society (2005)
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)
Sub-surface convection zones in hot massive stars and their observable consequences
M Cantiello;N Langer;N Langer;I Brott;A de Koter;A de Koter.
Astronomy and Astrophysics (2009)
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)
Quantitative Spectroscopy of O Stars at Low Metallicity: O Dwarfs in NGC 346*
J.-C. Bouret;T. Lanz;T. Lanz;D. J. Hillier;S. R. Heap.
The Astrophysical Journal (2003)
A New Spectral Classification System for the Earliest O Stars: Definition of Type O2
Nolan R. Walborn;Nolan R. Walborn;Ian D. Howarth;Daniel J. Lennon;Philip Massey;Philip Massey.
The Astronomical Journal (2002)
The VLT-FLAMES Tarantula Survey: I. Introduction and observational overview⋆
Chris Evans;W. D. Taylor;V. Hénault-brunet;H. Sana.
Astronomy and Astrophysics (2011)
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