Search Results - "Montmerle, Thierry"
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Million-Degree Plasma Pervading the Extended Orion Nebula
Published in Science (American Association for the Advancement of Science) (18-01-2008)“…Most stars form as members of large associations within dense, very cold (10 to 100 kelvin) molecular clouds. The nearby giant molecular cloud in Orion hosts…”
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HIGH-ENERGY PROCESSES IN YOUNG STELLAR OBJECTS
Published in Annual review of astronomy and astrophysics (01-01-1999)“…Observational studies of low-mass stars during their early stages of evolution, from protostars through the zero-age main sequence, show highly elevated levels…”
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3
A personal tribute to Pierre Valiron: scientist, thinker, man
Published in EPJ Web of conferences (01-01-2012)“…Pierre Valiron was “a great scientist, a great thinker, a great man”, prematurely taken away from us. His spirit lives, and his legacy, both scientific and…”
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ROSAT X-ray sources embedded in the rho Ophiuchi cloud core
Published in The Astrophysical journal (01-02-1995)Get full text
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5
Runaway O-star Bow Shocks as Particle Accelerators? The Case of AE Aur Revisited
Published in The Astrophysical journal (10-11-2019)“…We present results of our Chandra/ACIS observations of the field centered on the fast, runaway O star AE Aur and its bow shock. Previous XMM-Newton…”
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6
Gamma rays from active regions in the galaxy: The possible contribution of stellar winds
Published in Space science reviews (01-10-1983)“…A fraction of the mechanical energy released by stars larger than 20 solar masses in the form of strong stellar winds may be transferred to relativistic cosmic…”
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10 MK Gas in M17 and the Rosette Nebula: X-Ray Flows in Galactic H II Regions
Published in The Astrophysical journal (20-08-2003)Get full text
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Rotation and X-Ray Emission from Protostars
Published in The Astrophysical journal (01-04-2000)Get full text
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The role of accretion disks in the coronal activity of young stars
Published in Advances in space research (01-09-2003)“…X-ray observations have shown that, like all late-type stars, young, low-mass stars are magnetized. X-ray flaring characteristics suggest that the resulting…”
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3. Solar System Formation and Early Evolution: the First 100 Million Years
Published in Earth, moon, and planets (01-06-2006)“…The solar system, as we know it today, is about 4.5 billion years old. It is widely believed that it was essentially completed 100 million years after the…”
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Quasi-periodic X-Ray Flares from the Protostar YLW 15
Published in The Astrophysical journal (01-04-2000)Get full text
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12
Irradiation phenomena in young solar-type stars and the early solar system: X-ray observations and γ-ray constraints
Published in New astronomy reviews (01-07-2002)“…The high levels of X-ray flaring activity observed in young stars and protostars suggest correspondingly high levels of low-energy particle irradiation of…”
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Observations of supernova remnants and molecular clouds from the mm to the gamma-ray domain: bridging low and high energy cosmic rays
Published 07-10-2015“…New evidence that cosmic rays (hadronic component) are accelerated by supernova remnant shocks all the way from low energies to high energies, has come from…”
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14
A Stellar Merry-Go-Round
Published in Science (American Association for the Advancement of Science) (28-09-2001)“…Theoretical studies have predicted for some time that gaseous tori should exist around magnetic stars, as a result of the confinement of a stellar wind within…”
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On the Periodic X-Ray Emission from θ[TSUP]1[/TSUP] Orionis C
Published in The Astrophysical journal (10-08-1997)Get full text
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Comparing the spatial and kinematic distribution of gas and young stars around the shell-like structure in the CMa OB1 association
Published 18-08-2021“…A&A 654, A150 (2021) The relationship between young stellar clusters and respective parental molecular clouds is still an open issue: for instance, are the…”
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Gamma-rays from star-forming regions: from SNOBs to dark accelerators
Published 01-09-2009“…Observational gamma-ray astronomy was born some forty years ago, when small detectors were flown in satellites, following a decade of theoretical predictions…”
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Runaway O-star Bow Shocks as Particle Accelerators? The Case of AE Aur revisited
Published 03-09-2019“…We present results of our Chandra/ACIS observations of the field centered on the fast, runaway O star AE Aur and its bow shock. Previous XMM-Newton…”
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19
X-Ray-emitting T Tauri Stars in the L1551 Cloud
Published in The Astrophysical journal (10-06-1996)Get full text
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20
Cosmic ray induced ionisation of a molecular cloud shocked by the W28 supernova remnant
Published 03-07-2014“…A&A 568, A50 (2014) Cosmic rays are an essential ingredient in the evolution of the interstellar medium, as they dominate the ionisation of the dense molecular…”
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