Leutenegger, Maurice A.

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  1. Cohen D, Wollman E, Leutenegger M, Sundqvist J, Fullerton A, Zsargo J, Owocki S. MEASURING MASS-LOSS RATES AND CONSTRAINING SHOCK PHYSICS USING X-RAY LINE PROFILES OF O STARS FROM THE CHANDRA ARCHIVE. Mon. Not. Roy. Astron. Soc. 2014;439 (1):908-923.
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  2. Leutenegger M, Betancourt-Martinez G, Beiersdorfer P, Brown G, Kelley R, Kilbourne C, Porter F. CHARGE EXCHANGE MEASUREMENTS WITH AN X-RAY CALORIMETER AT AN ELECTRON BEAM ION TRAP. Phys. Scr. 2013;T156 4.
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  3. Leutenegger M, Cohen D, Sundqvist J, Owocki S. CONSTRAINTS ON POROSITY AND MASS LOSS IN O-STAR WINDS FROM MODELING OF X-RAY EMISSION LINE PROFILE SHAPES (VOL 770, PG 80, 2013). Astrophys. J. 2013;777 (1):1.
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  4. Leutenegger M, Cohen D, Sundqvist J, Owocki S. CONSTRAINTS ON POROSITY AND MASS LOSS IN O-STAR WINDS FROM THE MODELING OF X-RAY EMISSION LINE PROFILE SHAPES. Astrophys. J. 2013;770 (1):17.
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  5. Brown G, Beilmann C, Bernitt S, Clementson J, Eberle S, Epp S, Graf A, Hell N, Kelley R, Kilbourne C, Kubicek K, Leutenegger M, Maeckel V, Porter F, Rudolph J, Simon M, Steinbruegge R, Traebert E, Ullrich J, Lopez-Urrutia J, Beiersdorfer P. STUDIES OF HIGHLY CHARGED IRON IONS USING ELECTRON BEAM ION TRAPS FOR INTERPRETING ASTROPHYSICAL SPECTRA. Phys. Scr. 2013;T156 3.
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  6. Rudolph J, Bernitt S, Epp S, Steinbruegge R, Beilmann C, Brown G, Eberle S, Graf A, Harman Z, Hell N, Leutenegger M, Mueller A, Schlage K, Wille H, Yavas H, Ullrich J, Lopez-Urrutia J. X-RAY RESONANT PHOTOEXCITATION: LINEWIDTHS AND ENERGIES OF K ALPHA TRANSITIONS IN HIGHLY CHARGED FE IONS. Phys. Rev. Lett. 2013;111 (10):6.
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  7. Leutenegger M, Cohen D, Owocki S. ATOMIC PHYSICS OF SHOCKED PLASMA IN WINDS OF MASSIVE STARS. In: 17TH INTERNATIONAL CONFERENCE ON ATOMIC PROCESSES IN PLASMAS (ICAPIP). 17th International Conference on Atomic Processes in Plasmas (ICAPiP); JUL 19-22, 2011; Belfast, NORTH IRELAND. 2012. p. 111-117.
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  8. Sundqvist J, Owocki S, Cohen D, Leutenegger M, Townsend R. GENERALIZED POROSITY FORMALISM FOR ISOTROPIC AND ANISOTROPIC EFFECTIVE OPACITY AND ITS EFFECTS ON X-RAY LINE ATTENUATION IN CLUMPED O STAR WINDS. Mon. Not. Roy. Astron. Soc. 2012;420 (2):1553-1561.
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  9. Beiersdorfer P, Brown G, Graf A, Bitter M, Hill K, Kelley R, Kilbourne C, Leutenegger M, Porter F. REST-WAVELENGTH FIDUCIALS FOR THE ITER CORE IMAGING X-RAY SPECTROMETER. Rev. Sci. Instrum. 2012;83 (10):3.
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  10. Bernitt S, Brown G, Rudolph J, Steinbruegge R, Graf A, Leutenegger M, Epp S, Eberle S, Kubicek K, Maeckel V, Simon M, Traebert E, Magee E, Beilmann C, Hell N, Schippers S, Mueller A, Kahn S, Surzhykov A, Harman Z, Keitel C, Clementson J, Porter F, Schlotter W, Turner J, Ullrich J, Beiersdorfer P, Lopez-Urrutia J. UNEXPECTEDLY LOW OSCILLATOR STRENGTH AS THE ORIGIN OF THE FE XVII EMISSION PROBLEM. Nature. 2012;492 (7428):225-228.
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  11. Cohen D, Gagne M, Leutenegger M, MacArthur J, Wollman E, Sundqvist J, Fullerton A, Owocki S. CHANDRA X-RAY SPECTROSCOPY OF THE VERY EARLY O SUPERGIANT HD 93129A: CONSTRAINTS ON WIND SHOCKS AND THE MASS-LOSS RATE. Mon. Not. Roy. Astron. Soc. 2011;415 (4):3354-3364.
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  12. Cohen D, Leutenegger M, Wollman E, Zsargo J, Hillier D, Townsend R, Owocki S. MASS-LOSS RATE DETERMINATION FOR ZETA PUPPIS FROM THE QUANTITATIVE ANALYSIS OF X-RAY EMISSION-LINE PROFILES. Mon. Not. Roy. Astron. Soc. 2010;405 (4):2391-2405.
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  13. Leutenegger M, Beiersdorfer P, Brown G, Kelley R, Kilbourne C, Porter F. MEASUREMENT OF ANOMALOUSLY STRONG EMISSION FROM THE 1S-9P TRANSITION IN THE SPECTRUM OF H-LIKE PHOSPHORUS FOLLOWING CHARGE EXCHANGE WITH MOLECULAR HYDROGEN. Phys. Rev. Lett. 2010;105 (6):4.
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  14. Leutenegger M, Cohen D, Zsargo J, Martell E, MacArthur J, Owocki S, Gagne M, Hillier D. MODELING BROADBAND X-RAY ABSORPTION OF MASSIVE STAR WINDS. Astrophys. J. 2010;719 (2):1767-1774.
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  15. Zsargo J, Hillier D, Bouret J, Lanz T, Leutenegger M, Cohen D. ON THE IMPORTANCE OF THE INTERCLUMP MEDIUM FOR SUPERIONIZATION: O VI FORMATION IN THE WIND OF ZETA PUPPIS. Astrophys. J. Lett. 2008;685 (2):L149-L152.
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