Researcher Portfolio
Carlomagno, T.
Research Group of Liquid NMR Spectroscopy, MPI for biophysical chemistry, Max Planck Society
Researcher Profile
Position: Research Group of Liquid NMR Spectroscopy, MPI for biophysical chemistry, Max Planck Society
Researcher ID: https://pure.mpg.de/cone/persons/resource/persons14925
Publications
: Dessart, L., Ryu, T., Seoane, P. A., & Taylor, A. M. (2024). Light curves and spectra for theoretical models of high-velocity red-giant star collisions. ASTRONOMY & ASTROPHYSICS, 682: A58. doi:10.1051/0004-6361/202348228. [PubMan] : Dessart, L., & Hillier, D. J. (2006). Quantitative spectroscopic analysis of and distance to SN1999em. Astronomy & Astrophysics, 447(2), 691-707. doi:10.1051/0004-6361:20054044. [PubMan] : Dessart, L., & Hillier, D. J. (2005). Distance determinations using type II supernovae and the expanding photosphere method. Astronomy & Astrophysics, 439(2), 671-685. doi:10.1051/0004-6361:20053217. [PubMan] : Dessart, L., & Hillier, D. J. (2005). Quantitative spectroscopy of photospheric-phase type II supernovae. Astronomy & Astrophysics, 437(2), 667-685. doi:10.1051/0004-6361:20042525. [PubMan] : Dessart, L., & Owocki, S. P. (2005). 2D simulations of the line-driven instability in hot-star winds. Astronomy & Astrophysics, 437(2), 657-666. doi:10.1051/0004-6361:20052778. [PubMan] : Dessart, L., & Owocki, S. P. (2005). Inferring hot-star-wind acceleration from line profile variability. Astronomy & Astrophysics, 432(1), 281-294. doi:10.1051/0004-6361:20041461. [PubMan] : Dessart, L., & Hillier, D. J. (2005). Quantitative spectroscopy of type II supernovae. In M. Turatto, S. Benetti, L. Zampieri, & W. Shea (Eds. ), 1604-2004: Supernovae as cosmological lighthouses: Proceedings of a meeting held in Palazzo del Bo, Università degli Studi di Padova (pp. 401-402). San Francisco, CA, USA: Astronomical Society of the Pacific. [PubMan] : Dessart, L., & Hillier, D. J. (2005). Quantitative spectroscopy of type II supernovae with CMFGEN. In R. Humphreys K.Z. Stanek (Ed. ), The Fate of the Most Massive Stars (pp. 415-415). San Fransisco, CA, USA: Astronomical Society of the Pacific. [PubMan] : Dessart, L. (2004). 3D hydrodynamical simulations of corotating interaction regions in rotating line-driven stellar winds. Astronomy & Astrophysics, 423(2), 693-704. doi:10.1051/0004-6361:20040543. [PubMan] : Abbott, B., Crowther, P. A., Drissen, L., Dessart, L., Martin, P., & Boivin, G. (2004). Wolf-Rayet stars in M33 - I. Optical spectroscopy using CFHT-MOS. Monthly Notices of the Royal Astronomical Society, 350(2), 552-564. doi:10.1111/j.1365-2966.2004.07663.x. [PubMan] : Dessart, L. (2004). Structure and dynamics of hot star winds. In M. Heydari-Malayeri, P. Stee, & J.-P. Zahn (Eds. ), Evolution of Massive Stars, Mass Loss and Winds (pp. 251-270). Les Ulis, France: EDP Sciences. [PubMan] : Dessart, L., & Owocki, S. P. (2003). Two-dimensional simulations of the line-driven instability in hot-star winds. Astronomy & Astrophysics, 406(1), L1-L4. [PubMan] : Dessart, L., Langer, N., & Petrovic, J. (2003). The impact of radiation and wind momenta on mass transfer in massive close binary systems. Astronomy & Astrophysics, 404(3), 991-996. [PubMan]