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==== HEAD Meeting 2016 Special Session 201, Talks ==== | ==== HEAD Meeting 2016 Special Session 201, Talks ==== | ||
− | + | 201.01: [[Media:head.mtw.overview.july252016.website_small.pdf|Accretion Powered X-ray pulsars: Physics of the accretion column]]\\ Michael T. Wolff (NRL) | |
− | * 201.02: | + | * 201.02: [[Media:dianacheatham_head_2016_presentation.pdf|Application of a physical continuum model to recent X-ray observations of accreting pulsars]]\\ Diana M. Marcu-Cheatham (UMBC & NASA-GSFC) |
− | * 201.03: | + | * 201.03: [[Media:crsf.pdf|Cyclotron lines]]\\ Jörn Wilms (Remeis Observatory, FAU) |
− | * 201.04: | + | * 201.04: [[Media:spelum.pdf|Spectrum-luminosity dependence of radiation from polar emitting regions in accreting magnetized neutron stars]]\\ Dmitry Klochkov (IAA Tübingen) |
− | * 201.05: | + | * 201.05: [[Media:201.05_staubert.pdf|Long-term change in the cyclotron line energy in Hercules X-1]]\\ Rüdiger Staubert (IAA Tübingen) |
− | * 201.06: | + | * 201.06: [[Media:hemphill_head2016_talk.pdf|Evidence for an evolving cyclotron line energy in 4U 1538-522]]\\ Paul B. Hemphill (CASS-UCSD) |
− | * 201.07: | + | * 201.07: [[Media:head_naples_nustar_pulsars.pdf|Pulsar observations with NuSTAR]]\\ Felix Fürst (Caltech) |
− | * 201.08: | + | * 201.08: [[Media:201604_head.pdf|Self-consistent accretion column modeling]]\\ Sebastian Falkner (Remeis Observatory, FAU) |
==== Related Poster Presentations ==== | ==== Related Poster Presentations ==== |
Revision as of 15:30, 25 June 2018
HEAD Meeting 2016 Special Session 201, Talks
201.01: Accretion Powered X-ray pulsars: Physics of the accretion column\\ Michael T. Wolff (NRL)
* 201.02: Application of a physical continuum model to recent X-ray observations of accreting pulsars\\ Diana M. Marcu-Cheatham (UMBC & NASA-GSFC)
* 201.03: Cyclotron lines\\ Jörn Wilms (Remeis Observatory, FAU)
* 201.04: Spectrum-luminosity dependence of radiation from polar emitting regions in accreting magnetized neutron stars\\ Dmitry Klochkov (IAA Tübingen)
* 201.05: Long-term change in the cyclotron line energy in Hercules X-1\\ Rüdiger Staubert (IAA Tübingen)
* 201.06: Evidence for an evolving cyclotron line energy in 4U 1538-522\\ Paul B. Hemphill (CASS-UCSD)
* 201.07: Pulsar observations with NuSTAR\\ Felix Fürst (Caltech)
* 201.08: Self-consistent accretion column modeling\\ Sebastian Falkner (Remeis Observatory, FAU)
Related Poster Presentations
* 120.03: Head16:poster bodaghee small.pdf\\ Arash Bodaghee (Georgia College)
* 120.06: Head16:brumbackheadposter.pdf\\ McKinley C. Brumback (Dartmouth College)
* 120.09: Head16:cenx3b.pdf\\ Amy M. Gottlieb (Univ. Florida & UMBC & NASA-GSFC)
* 120.21: Head16:gx304 poster3.pdf\\ Richard E. Rothschild (CASS-UCSD)
* 120:24: Head16:head.herx1.poster.v2.mar312016.pdf\\ Michael T. Wolff (NRL)