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Massive star

The VLT-FLAMES Tarantula Survey. XXIX. Massive star formation in the local 30 Doradus starburst

The VLT-FLAMES Tarantula Survey. XXIX. Massive star formation in the local 30 Doradus starburst

... of massive stars in 30 Dor using masses and ages derived for 452 mainly OB stars from the spectroscopic VLT-FLAMES Tarantula Survey ...that massive stars either moved large distances or formed independently ...

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New results on the massive star-forming region S106 by BEAR spectro-imagery

New results on the massive star-forming region S106 by BEAR spectro-imagery

... a massive star with its parent cloud, the close environment of S106 IR in the star-forming region S106 was observed at high spectral resolution ( ∼16 km s −1 ...

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The formation and evolution of massive star clusters: historical overview

The formation and evolution of massive star clusters: historical overview

... of star clusters and cluster ...active star formation just outside their ...super star clusters in own Milky Way ...of massive star clusters is favored in a region where differential ...

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3D modelling of the massive star binary systems Eta Carinae, WR 22, and WR 140

3D modelling of the massive star binary systems Eta Carinae, WR 22, and WR 140

... Abstract: Massive stars possess powerful stellar ...a massive star binary system generates a region of thermalized plasma which may emit prolifically at X-ray ...

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Deviations from a uniform period spacing of gravity modes in a massive star

Deviations from a uniform period spacing of gravity modes in a massive star

... a massive star Pieter Degroote 1 , Conny Aerts 1,2 , Annie Baglin 3 , Andrea Miglio 4 , Maryline Briquet 1 , Arlette Noels 4 , Ewa Niemczura 5 , Josefina Montalban 4 , Steven Bloemen 1 , Raquel Oreiro 1 , ...

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Characterizing filaments in regions of high-mass star formation: High-resolution submilimeter imaging of the massive star-forming complex NGC 6334 with ArT\'eMiS

Characterizing filaments in regions of high-mass star formation: High-resolution submilimeter imaging of the massive star-forming complex NGC 6334 with ArT\'eMiS

... more massive than these filaments, respectively (see Table 1 ...in massive star-forming complexes, is based on multiple episodes of large-scale supersonic com- pression due to interaction of ...

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The formation and evolution of massive star clusters: historical overview

The formation and evolution of massive star clusters: historical overview

... numerous star clusters and as- sociations, this indicated that strong tidal interactions and mergers can trigger bursts of cluster ...of massive star clusters ...all star formation that takes ...

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Triggered massive-star formation on the borders of Galactic HII regions Evidence for the collect and collapse process around RCW 79

Triggered massive-star formation on the borders of Galactic HII regions Evidence for the collect and collapse process around RCW 79

... of massive star formation at the bor- ders of RCW ...of massive-star formation may still be present, represent- ing ideal sites to address the question of massive star ...

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A new hybrid radiative transfer method for massive star formation

A new hybrid radiative transfer method for massive star formation

... of massive star formation, the flashlight effect is due to the nonisotropic character of the radiation field because the opti- cal thickness is very different in the disk direction and in the cavities ...

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Solar-Like Oscillations in a Massive Star

Solar-Like Oscillations in a Massive Star

... Seismology of stars provides insight into the physical mechanisms taking place in their interior, with modes of oscillation probing different layers. Low-amplitude acoustic oscillations excited by turbulent convection ...

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Colliding-winds in massive star binaries: expectations from radio to gamma-rays

Colliding-winds in massive star binaries: expectations from radio to gamma-rays

... Emission processes Emission processes What is expected in the visible domain? What is expected in the visible domain? ­ globally, visible spectra are populated by only a few lines ­ g[r] ...

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The Herschel view of the massive star-forming region NGC 6334

The Herschel view of the massive star-forming region NGC 6334

... In the scenario described above, one would expect that sub- regions within one molecular cloud complex may be in different states with regard to turbulence and gravity, i.e., star-forming versus ...

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Spectroscopy of Massive Stars

Spectroscopy of Massive Stars

... are smoothed out over the whole emitting volume, leading to a rather constant X-ray output (Feldmeier et al. 1997). In addition, a supple- mentary X-ray emission may result from other mechanisms, which are not ...

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Star Wars : l'Empire de la désillusion

Star Wars : l'Empire de la désillusion

... occupe. Star Wars expose une vision largement manichéenne de la morale : le bien versus le mal, la lumière contre l’obscurité, qui composent les deux faces de ce qui s’y nomme « la force », en- tité immatérielle ...

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Star Coloring of Graphs

Star Coloring of Graphs

... a star coloring with k ...the star chromatic number of different families of graphs such as trees, cycles, complete bipartite graphs, outerplanar graphs and 2-dimensional ...the star chromatic number ...

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Une lecture politique de Star trek /

Une lecture politique de Star trek /

... facon de falre peut nous rappeler les mythes qui transcendent les découverte~ des slècles passés. MalS dans le contexte amérl- caln, cette mythologle n'a pas de c[r] ...

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Massive Gravity on a Brane

Massive Gravity on a Brane

... 1 Introduction Recently there has been considerable interest in theories of gravitation which deviate from Einstein’s gravity at very long distances (for example, [1–5]). However there has been no consistent theory yet ...

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Precise radial velocities of giant stars IX. HD 59686 Ab: a massive circumstellar planet orbiting a giant star in a \~13.6 au eccentric binary system

Precise radial velocities of giant stars IX. HD 59686 Ab: a massive circumstellar planet orbiting a giant star in a \~13.6 au eccentric binary system

... The only unsaturated photometry for HD 59686 A was ac- quired by the Hipparcos mission ( ESA 1997 ) between March 16 th 1990 and March 10 th 1993 (2447966.9 – 2449057.2 JD), more than 6 years before first RV observations ...

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Réfection des murs de maçonnerie massive

Réfection des murs de maçonnerie massive

... / La version de cette publication peut être l’une des suivantes : la version prépublication de l’auteur, la version acceptée du manuscrit ou la version de l’éditeur. Access and use of [r] ...

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Signaux qualitatifs et phénomène de star

Signaux qualitatifs et phénomène de star

... de star peut exister même en l’absence de talent : il est le résultat du hasard et de la stratégie de minimisation des coûts d’information mise en œuvre par les ...de star, ils se placent explicitement sur ...

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