activity
20042016
most citedMY Camelopardalis, a very massive merger progenitor

21 citations · 113 across the 20 of their papers we have counts for

collaborators

20 papers

astro-ph.EP2016★ 6 cited

Properties of interstellar wind leading to shape morphology of the dust surrounding HD 61005

P. Pastor

A structure formed by dust particles ejected from the debris ring around HD 61005 is observed in the scattered light. The main aim here is to constrain interstellar wind parameters…

astro-ph.SR2016★ 12 cited

GU Mon, a high-mass eclipsing overcontact binary in the young open cluster Dolidze 25

J. Lorenzo, I. Negueruela, F. Vilardell +3

Context. The eclipsing binary GU Mon is located in the star-forming cluster Dolidze 25, which has the lowest metallicity measured in a Milky Way young cluster. Aims. GU Mon has bee…

astro-ph.EP2015

Linearized averaged resonant equations and their solution for dust particles

Pavol Pastor

The averaged resonant equations of motion for the planar circular restricted three-body problem are solved on the linearization basis taking into account also non-gravitational eff…

astro-ph.EP2015★ 5 cited

Locations of stationary/periodic solutions in mean motion resonances according to properties of dust grains

Pavol Pastor

The equations of secular evolution for dust grains in mean motion resonances with a planet are solved for stationary points. This is done including both Poynting-Robertson effect a…

astro-ph.SR2014★ 21 cited

MY Camelopardalis, a very massive merger progenitor

J. Lorenzo, I. Negueruela, A. K. F. Val Baker +4

Context. The early-type binary MY Cam belongs to the young open cluster Alicante 1, embedded in Cam OB3. Aims. MY Cam consists of two early-O type main-sequence stars and shows a p…

astro-ph.EP2014★ 5 cited

Positions of equilibrium points for dust particles in the circular restricted three-body problem with radiation

P. Pastor

For a body with negligible mass moving in the gravitational field of a star and one planet in a circular orbit (the circular restricted three-body problem) five equilibrium points…