THE CLOSE T TAURI BINARY SYSTEM V4046 Sgr: ROTATIONALLY MODULATED X-RAY EMISSION FROM ACCRETION SHOCKS
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Title
THE CLOSE T TAURI BINARY SYSTEM V4046 Sgr: ROTATIONALLY MODULATED X-RAY EMISSION FROM ACCRETION SHOCKS
Authors
Keywords
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Journal
ASTROPHYSICAL JOURNAL
Volume 752, Issue 2, Pages 100
Publisher
IOP Publishing
Online
2012-06-01
DOI
10.1088/0004-637x/752/2/100
References
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Related references
Note: Only part of the references are listed.- TW Hya: SPECTRAL VARIABILITY, X-RAYS, AND ACCRETION DIAGNOSTICS
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- GSC 07396-00759 = V4046 Sgr C[D]: A WIDE-SEPARATION COMPANION TO THE CLOSE T TAURI BINARY SYSTEM V4046 Sgr AB
- (2011) J. H. Kastner et al. Astrophysical Journal Letters
- Modelling circumbinary gas flows in close T Tauri binaries★
- (2011) M. de Val-Borro et al. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- The close classical T Tauri binary V4046 Sgr: complex magnetic fields and distributed mass accretion
- (2011) J.-F. Donati et al. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- On the observability of T Tauri accretion shocks in the X-ray band
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- (2010) R. L. Curran et al. ASTRONOMY & ASTROPHYSICS
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- (2010) David R. Rodriguez et al. ASTROPHYSICAL JOURNAL
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- (2010) J.-F. Donati et al. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- X-ray optical depth diagnostics of T Tauri accretion shocks
- (2009) C. Argiroffi et al. ASTRONOMY & ASTROPHYSICS
- X-ray spectroscopy of stars
- (2009) Manuel Güdel et al. ASTRONOMY AND ASTROPHYSICS REVIEW
- Molecules in the disk orbiting the twin young suns of V4046 Sagittarii
- (2008) J. H. Kastner et al. ASTRONOMY & ASTROPHYSICS
- X-ray emission from dense plasma in classical T Tauri stars: hydrodynamic modeling of the accretion shock
- (2008) G. G. Sacco et al. ASTRONOMY & ASTROPHYSICS
- PHOTOEVAPORATION OF CIRCUMSTELLAR DISKS BY FAR-ULTRAVIOLET, EXTREME-ULTRAVIOLET AND X-RAY RADIATION FROM THE CENTRAL STAR
- (2008) U. Gorti et al. ASTROPHYSICAL JOURNAL
- X‐Ray–Irradiated Protoplanetary Disk Atmospheres. I. Predicted Emission‐Line Spectrum and Photoevaporation
- (2008) Barbara Ercolano et al. ASTROPHYSICAL JOURNAL
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