Zobrazeno 1 - 10
of 171
pro vyhledávání: '"C. M. Boily"'
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 644, pp.A141. ⟨10.1051/0004-6361/202039118⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 644, pp.A141. ⟨10.1051/0004-6361/202039118⟩
Astronomy and Astrophysics-A&A, 2020, 644, pp.A141. ⟨10.1051/0004-6361/202039118⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 644, pp.A141. ⟨10.1051/0004-6361/202039118⟩
Young stellar clusters harbour complex spatial structures emerging from the star formation process. Identifying stellar over-densities is a key step to constrain better how these structures are formed. The high accuracy of distances derived from Gaia
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 465 (2), pp.2198-2211. ⟨10.1093/mnras/stw2880⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 465 (2), pp.2198-2211. ⟨10.1093/mnras/stw2880⟩
International audience; We explore with collisional gravitational N-body models the evolution of binary stars in initially fragmented and globally subvirial clusters of stars. Binaries are inserted in the (initially) clumpy configurations so as to ma
Autor:
Julien Dorval, C. M. Boily
Publikováno v:
Proceedings of the International Astronomical Union. 12:246-250
Stellar clusters form with a high level of substructure, inherited from the molecular cloud and the star formation process. Evidence from observations and simulations also indicate the stars in such young clusters form a subvirial system. The subsequ
Autor:
C. M. Boily
Publikováno v:
Gravity and the Quantum ISBN: 9783319516998
The motion of a black hole (BH) about the centre of gravity of its host galaxy induces a strong response from the surrounding stars. We revisit the case of a harmonic potential and argue that half of the stars on circular orbits in that potential shi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c8470faf692bb46021de602f24c96efb
https://doi.org/10.1007/978-3-319-51700-1_3
https://doi.org/10.1007/978-3-319-51700-1_3
Autor:
C. M. Boily, Benoit Famaey, Giacomo Monari, Robert J. J. Grand, Arnaud Siebert, Daisuke Kawata
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 461 (4), pp.3835-3846. ⟨10.1093/mnras/stw1564⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 461 (4), pp.3835-3846. ⟨10.1093/mnras/stw1564⟩
We investigate models of the Milky Way disc taking into account simultaneously the bar and a two-armed quasi-static spiral pattern. Away from major resonance overlaps, the mean stellar radial motions in the plane are essentially a linear superpositio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2e99f586569d7102ab7a91667bdab736
https://hal.archives-ouvertes.fr/hal-03144476/file/stw1564.pdf
https://hal.archives-ouvertes.fr/hal-03144476/file/stw1564.pdf
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 459 (2), pp.1213-1232. ⟨10.1093/mnras/stw714⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 459 (2), pp.1213-1232. ⟨10.1093/mnras/stw714⟩
This paper discusses a new method to generate self-coherent initial conditions for young substructured stellar cluster. The expansion of a uniform system allows stellar sub-structures (clumps) to grow from fragmentation modes by adiabatic cooling. We
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c051e2b6332ee8f79f1c1d80a23aa58d
http://arxiv.org/abs/1603.07223
http://arxiv.org/abs/1603.07223
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 418:759-769
We present a novel and flexible tensor approach to computing the effect of a time-dependent tidal field acting on a stellar system. The tidal forces are recovered from the tensor by polynomial interpolation in time. The method has been implemented in
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 407:2122-2130
We find that a steady state bar induces transient features at low velocities in the solar neighborhood velocity distribution due to the initial response of the disc, following the formation of the bar. We associate these velocity streams with two qua
Autor:
Simon J. Karl, Florent Renaud, Peter H. Johansson, Thorsten Naab, C. M. Boily, Christian Theis, Hanna Kotarba
Publikováno v:
The Astrophysical Journal. 715:L88-L93
We present a new high-resolution N-body/SPH simulation of an encounter of two gas-rich disk galaxies which closely matches the morphology and kinematics of the interacting Antennae galaxies (NGC 4038/39). The simulation includes radiative cooling, st
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 401:1898-1903
This paper introduces a novel approach for sampling the orbits of an N-body simulation. The gist of the method is to exploit individual phase-space coordinates acquired during integration of the equations of motion. This technique, which we dub ‘pa