Moffat, A.F.J.
Anthony Moffat astronomer
Moffat, Anthony F.J.
Moffat, Anthony
Moffat, A.F.J. (Anthony F.J.)
VIAF ID: 44390794 (Personal)
Permalink: http://viaf.org/viaf/44390794
Preferred Forms
- 100 0 _ ‡a Anthony Moffat ‡c astronomer
- 200 _ | ‡a Moffat ‡b Anthony F. J.
-
-
-
- 100 1 0 ‡a Moffat, A. F. J.
- 100 1 _ ‡a Moffat, A. F. J.
- 100 1 _ ‡a Moffat, A.F.J.
-
-
-
-
- 100 1 _ ‡a Moffat, Anthony F.J.
4xx's: Alternate Name Forms (18)
Works
Title | Sources |
---|---|
BRITE observations of classical Cepheids : an update | |
ETA CARINAE’S THERMAL X-RAY TAIL MEASURED WITHXMM-NEWTONANDNuSTAR | |
Etude de la variabilité des étoiles massives à l'aide de la photométrie et de la spectroscopie | |
Four Decades of Research on Massive Stars : [proceedings from a scientific meeting in honor of Anthony F.J. Moffat held at Auberge du Lac Taureau, St-Michel-des-Saints, Québec, Canada, 11-15 July 2011] | |
Instability and variability of hot-star winds, 1995: | |
An introduction to the Chandra Carina complex project | |
Massive stars in interacting binaries : proceedings of a workshop held at Hotel Sacacomie, Mauricie, Québec, Canada, 16-20 August 2004 | |
MOST detects transits of HD 97658b, a warm, likely volatile-rich super-earth | |
The MOST view of Cepheids | |
A near-infrared survey of the inner Galactic plane for Wolf-Rayet stars - III. New methods: faintest WR stars | |
NGC 1624-2: a slowly rotating, X-ray luminous Of?cp star with an extraordinarily strong magnetic field | |
NON-DETECTION OF PREVIOUSLY REPORTED TRANSITS OF HD 97658b WITHMOSTPHOTOMETRY | |
Non-equilibrium radiative hypersonic flows: theoretical, observational and numerical aspects in astrophysics and aerospace industry : proceedings of the 5th Workshop of the GDR "Milieux Circumstellaires" of the CNRS (France), with the Universities of Strasbourg and Montreal held in Mont Sainte Odile, France, 22-25 September, 1997 | |
Non-thermal X-rays from colliding wind shock acceleration in the massive binary Eta Carinae | |
Nonradial p-modes in the G9.5 giant ϵ Ophiuchi? Pulsation model fits to MOST photometry | |
Observing the massive binary η Carinae with BRITE | |
On the origin of mass segregation in NGC 3603 | |
On the origin of variable structures in the winds of hot luminous stars | |
THE Onfp CLASS IN THE MAGELLANIC CLOUDS | |
Optical spectroscopy of X-Mega targets - II. The massive double-lined O-type binary HD 93205 | |
The orbit and stellar masses of the archetype colliding-wind binary WR 140 | |
Orbitally modulated dust formation by the WC7+O5 colliding-wind binary WR140 | |
Outmoving Clumps in the Wind of the Hot O Supergiant ζ Puppis | |
Photometric variability in FU Ori and Z CMa as observed by MOST★ | |
Physics of luminous blue variables : proceedings of the 113th Colloquium of the International Astronomical Union, held at Val Morin, Québec Province, Canada, August 15-18, 1988 | |
Pulsations and outbursts in Be stars : small differences - big impacts | |
R144 revealed as a double-lined spectroscopic binary | |
Recent X-ray Activity of Eta Car as Seen by the Swift/XRT | |
Recherche systématique d'étoiles binaires parmi les étoiles Wolf-Rayet de sous-type spectral WNE dans les Nuages de Magellan | |
Reduction of time-resolved space-based CCD photometry developed for MOST Fabry Imaging data | |
Regular frequency patterns in the classicalδScuti star HD 144277 observed by the MOST satellite | |
Resolving Decades of Periodic Spirals from the Wolf–Rayet Dust Factory WR 112 | |
Resolving OB Systems in the Carina Nebula with theHubble Space TelescopeFine Guidance Sensor | |
Resolving X-ray emission in the galactic ``Starburst'' NGC 3603 with Chandra | |
A response to P.S. Conti's comment on "A three-dimensional classification for WN stars" | |
Rotation and magnetic activity of the Hertzsprung-gap giant 31 Comae | |
ROTATIONALLY MODULATEDg-MODES IN THE RAPIDLY ROTATING δ SCUTI STAR RASALHAGUE (α OPHIUCHI) | |
The search for low-mass companions of B stars in the Carina nebula cluster Trumpler 16 | |
A search for p-modes and other variability in the binary system 85 Pegasi using MOST photometry | |
Seismic modelling of early B-type pulsators observed by BRITE – I. θ Ophiuchi | |
Short-term variability and mass loss in Be stars | |
Space Photometry with Brite-Constellation | |
Spectroscopic and polarimetric parameters of the runaway WN7 binary system HD 197406 - Is the secondary an X-ray-quiet black hole? | |
Spectroscopic follow-up of the colliding-wind binary WR 140 during the 2009 January periastron passage | |
Spectroscopic study of the long-period dust-producing WC7pd+O9 binary HD 192641 | |
Spectroscopy,MOSTphotometry, and interferometry of MWC 314: is it an LBV or an interacting binary? | |
Stable and unstable accretion in the classical T Tauri stars IM Lup and RU Lup as observed byMOST | |
A stable quasi-periodic 4.18-d oscillation and mysterious occultations in the 2011 MOST light-curve of TW Hya | |
O Stars in Transition. I. Optical Spectroscopy of Ofpe/WN9 and Related Stars | |
Start of Eta Car's X-ray minimum | |
Stellar masses from granulation and oscillations of 23 bright red giants observed by BRITE-Constellation | |
Stellar Model Analysis of the Oscillation Spectrum of η Bootis Obtained fromMOST | |
Stellar modelling of Spica, a high-mass spectroscopic binary with a β Cep variable primary component | |
Study of the variability of massive stars using photometry and spectroscopy. | |
A systematic study of variability among OB-stars based on HIPPARCOS photometry | |
Système solaire et physique stellaire. (A. Moffat). | |
The Tarantula Massive Binary Monitoring | |
Towards the Albedo of an Exoplanet: MOST Satellite Observations of Bright Transiting Exoplanetary Systems | |
Triple system HD 201433 with a SPB star component seen by BRITE - Constellation: Pulsation, differential rotation, and angular momentum transfer | |
Turbulence in outflows from hot stars | |
Understanding the photometric variability of zeta Ori Aa | |
Unraveling the oldest and faintest recovered nova - CK Vulpeculae (1670) | |
An Upper Limit on the Albedo of HD 209458b: Direct Imaging Photometry with theMOSTSatellite | |
UsingMOSTto reveal the secrets of the mischievous Wolf-Rayet binary CV Ser | |
UW CMa : a questionable contact system | |
V473 Lyr, a modulated, period-doubled Cepheid, and U TrA, a double-mode Cepheid observed by MOST | |
Variability monitoring of OB stars during the Mons campaign | |
The Very Low Albedo of an Extrasolar Planet:MOSTSpace‐based Photometry of HD 209458 | |
VLT/SINFONI time-resolved spectroscopy of the central, luminous, H-rich WN stars of R136 | |
VLTI-AMBER velocity-resolved aperture-synthesis imaging ofηCarinae with a spectral resolution of 12 000 | |
Weighting the most massive stars | |
Wind Inhomogeneities in Wolf-Rayet Stars. IV. Using Clumps to Probe the Wind Structure in the WC8 Star HD 192103 | |
Wolf-Rayet stars with BRITE | |
ξTauri: a unique laboratory to study the dynamic interaction in a compact hierarchical quadruple system |