NewEvery arXiv paper, its researchers & institutions — mapped.
papers

Publications (13)

astro-ph.IM2014

A method to deconvolve stellar rotational velocities

Michel Cure, Diego F. Rial, Alejandra Christen +1

astro-ph.IM2014

A method to deconvolve mass ratio distribution from binary stars

Michel Cure, Diego F. Rial, Alejandra Christen +2

astro-ph2004

The influence of rotation in radiation driven winds from hot stars II. CAK topological analysis

Michel Cure, Diego Rial

astro-ph.SR2018

Imaging the disc rim and a moving close-in companion candidate in the pre-transitional disc of V1247 Orionis

Matthew Willson, Stefan Kraus, Jacques Kluska +17

astro-ph2007

A New Numerical Method for Solving Radiation Driven Winds from Hot Stars

Michel Cure, Diego F. Rial

astro-ph.EP2018

Differences in the gas and dust distribution in the transitional disk of a sun-like young star, PDS 70

Zachary C. Long, Eiji Akiyama, Michael Sitko +22

astro-ph.SR2013

Pulsations as a mass-loss trigger in evolved hot stars

Michaela Kraus, Dieter H. Nickeler, Maximiliano Haucke +5

astro-ph.SR2012

A cyclic bipolar wind in the interacting binary V393 Scorpii

Ronald Mennickent, Zbigniew Kolaczkowski, Ewa Niemczura +4

astro-ph.SR2014

Analytical Solutions for Radiation-Driven Winds in Massive Stars. I: The Fast Regime

Ignacio Araya, Michel Cure, Lydia S. Cidale

astro-ph.SR2012

Stars with the B[e] phenomenon seen by long baseline interferometry

Marcelo Borges Fernandes, Olivier Chesneau, Michaela Kraus +11

astro-ph.SR2011

Variability of Disk Emission in Pre-Main Sequence and Related Stars. II. Variability in the Gas and Dust Emission of the Herbig Fe Star SAO 206462

Michael L. Sitko, Amanda N. Day, Robin L. Kimes +16

astro-ph.SR2017

Resolving the circumstellar environment of the Galactic B[e] supergiant star MWC 137 from large to small scales

Michaela Kraus, Tiina Liimets, Cristina E. Cappa +10

astro-ph.SR2019

A method to deconvolve stellar rotational velocities III. The probability distribution function via Maximum Likelihood utilizing Finite Distribution Mixtures

Rafael Orellana, Pedro Escarate, Michel Cure +3