Joseph M. Neilsen, Ph.D.
Affiliations: | 2011 | Harvard University, Cambridge, MA, United States |
Area:
Astrophysics Physics, Astronomy and AstrophysicsGoogle:
"Joseph Neilsen"Mean distance: (not calculated yet)
Parents
Sign in to add mentor| Julia C. Lee | grad student | 2011 | Harvard | |
| (Winds of Change: The Physics of Accretion, Ejection, and Fast X-ray Variability in GRS 1915+105.) | ||||
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Publications
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| Wang J, Kara E, Steiner JF, et al. (2020) Relativistic Reflection and Reverberation in GX 339–4 with NICER and NuSTAR The Astrophysical Journal. 899: 44 |
| Rosa AD, Uttley P, Gou L, et al. (2018) Accretion in strong field gravity with eXTP Science China Physics, Mechanics & Astronomy. 62 |
| Zhang S, Baganoff FK, Ponti G, et al. (2017) Sagittarius ${\rm{A}}* $ High-energy X-Ray Flare Properties duringNuStarMonitoring of the Galactic Center from 2012 to 2015 The Astrophysical Journal. 843: 96 |
| Homan J, Neilsen J, Allen JL, et al. (2016) EVIDENCE FOR SIMULTANEOUS JETS AND DISK WINDS IN LUMINOUS LOW-MASS X-RAY BINARIES The Astrophysical Journal. 830: L5 |
| Heinz S, Corrales L, Smith R, et al. (2016) A Joint Chandra And Swift View Of The 2015 X-Ray Dust-Scattering Echo Of V404 Cygni The Astrophysical Journal. 825: 15 |
| Neilsen J, Rahoui F, Homan J, et al. (2016) A Super-Eddington, Compton-thick Wind in GRO J1655-40? The Astrophysical Journal. 822: 20 |
| Ponti G, De Marco B, Morris MR, et al. (2015) Fifteen years of XMM-Newton and Chandra monitoring of Sgr A*: Evidence for a recent increase in the bright flaring rate Monthly Notices of the Royal Astronomical Society. 454: 1525-1544 |
| Li YP, Yuan F, Yuan Q, et al. (2015) STATISTICS OF X-RAY FLARES OF SAGITTARIUS A∗: EVIDENCE FOR SOLAR-LIKE SELF-ORGANIZED CRITICALITY PHENOMENA Astrophysical Journal. 810 |
| Neilsen J, Coriat M, Fender R, et al. (2014) A link between X-ray emission lines and radio jets in 4U 1630-47? Astrophysical Journal Letters. 784 |
| Chakravorty S, Lee JC, Neilsen J. (2013) The effects of thermodynamic stability on wind properties in different low-mass black hole binary states Monthly Notices of the Royal Astronomical Society. 436: 560-569 |