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@article{hurst_longterm_1951,
title = {Long-term storage capacity of reservoirs},
volume = {116},
url = {http://www.citeulike.org/group/2384/article/7655765},
timestamp = {2015-11-21T14:17:24Z},
journal = {Transactions of the {American} {Society} of {Civil} {Engineers}},
shortjournal = {{T} {AM} {SOC} {CIV} {ENG}},
author = {Hurst, {Harold} {Edwin}},
urldate = {2015-11-18},
date = {1951},
pages = {770--808},
file = {Snapshot:/Users/mpwd/Library/Application Support/Zotero/Profiles/fk5ookxj.default/zotero/storage/UT6WE3AI/7655765.html:}
}
@book{taleb_silent_2015,
title = {Silent {Risk}},
url = {https://drive.google.com/file/d/0B8nhAlfIk3QIR1o1dnk5ZmRaaGs/view?pli=1},
timestamp = {2015-11-21T14:53:03Z},
author = {Taleb, {Nassim} {Nicholas}},
publisher = {Manuscript},
urldate = {2015-11-18},
date = {2015},
file = {Snapshot:/Users/mpwd/Library/Application Support/Zotero/Profiles/fk5ookxj.default/zotero/storage/SJ6HPIW6/view.html:}
}
@article{miller_flows_2015,
title = {Flows of {X}-ray gas reveal the disruption of a star by a massive black hole},
volume = {526},
rights = {© 2015 {Nature} {Publishing} {Group}, a division of {Macmillan} {Publishers} {Limited}. {All} {Rights} {Reserved}.},
issn = {0028-0836},
url = {http://www.nature.com/nature/journal/v526/n7574/full/nature15708.html},
doi = {10.1038/nature15708},
abstract = {Tidal forces close to massive black holes can violently disrupt stars that make a close approach. These extreme events are discovered via bright X-ray and optical/ultraviolet flares in galactic centres. Prior studies based on modelling decaying flux trends have been able to estimate broad properties, such as the mass accretion rate. Here we report the detection of flows of hot, ionized gas in high-resolution X-ray spectra of a nearby tidal disruption event, ASASSN-14li in the galaxy PGC 043234. Variability within the absorption-dominated spectra indicates that the gas is relatively close to the black hole. Narrow linewidths indicate that the gas does not stretch over a large range of radii, giving a low volume filling factor. Modest outflow speeds of a few hundred kilometres per second are observed; these are below the escape speed from the radius set by variability. The gas flow is consistent with a rotating wind from the inner, super-Eddington region of a nascent accretion disk, or with a filament of disrupted stellar gas near to the apocentre of an elliptical orbit. Flows of this sort are predicted by fundamental analytical theory and more recent numerical simulations.},
timestamp = {2015-11-19T17:58:27Z},
number = {7574},
journal = {Nature},
shortjournal = {Nature},
author = {Miller, {Jon} {M}. and {Kaastra}, {Jelle} {S}. and {Miller}, {M}. {Coleman} and {Reynolds}, {Mark} {T}. and {Brown}, {Gregory} and {Cenko}, {S}. {Bradley} and {Drake}, {Jeremy} {J}. and {Gezari}, {Suvi} and {Guillochon}, {James} and {Gultekin}, {Kayhan} and {Irwin}, {Jimmy} and {Levan}, {Andrew} and {Maitra}, {Dipankar} and {Maksym}, {W}. {Peter} and {Mushotzky}, {Richard} and {O}’{Brien}, {Paul} and {Paerels}, {Frits} and de {Plaa}, {Jelle} and {Ramirez}-{Ruiz}, {Enrico} and {Strohmayer}, {Tod} and {Tanvir}, {Nial}},
urldate = {2015-11-19},
date = {2015-10-22},
pages = {542--545},
langid = {english},
keywords = {High-energy astrophysics},
options = {useprefix},
file = {Snapshot:/Users/mpwd/Library/Application Support/Zotero/Profiles/fk5ookxj.default/zotero/storage/XUARZ4EP/nature15708.html:}
}
@article{boyajian_planet_2015,
title = {Planet {Hunters} {X}. {KIC} 8462852 - {Where}'s the {Flux}?},
url = {http://arxiv.org/abs/1509.03622},
abstract = {Over the duration of the Kepler mission, KIC 8462852 was observed to undergo irregularly shaped, aperiodic dips in flux down to below the 20\% level. The dipping activity can last for between 5 and 80 days. We characterize the object with high-resolution spectroscopy, spectral energy distribution fitting, and Fourier analyses of the Kepler light curve. We determine that KIC 8462852 is a main-sequence F3 V/IV star, with a rotation period {\textasciitilde}0.88 d, that exhibits no significant IR excess. In this paper, we describe various scenarios to explain the mysterious events in the Kepler light curve, most of which have problems explaining the data in hand. By considering the observational constraints on dust clumps orbiting a normal main-sequence star, we conclude that the scenario most consistent with the data is the passage of a family of exocomet fragments, all of which are associated with a single previous breakup event. We discuss the necessity of future observations to help interpret the system.},
timestamp = {2015-11-21T14:20:40Z},
journal = {Preprint},
shortjournal = {Preprint},
author = {Boyajian, {T}. {S}. and {LaCourse}, {D}. {M}. and {Rappaport}, {S}. {A}. and {Fabrycky}, {D}. and {Fischer}, {D}. {A}. and {Gandolfi}, {D}. and {Kennedy}, {G}. {M}. and {Liu}, {M}. {C}. and {Moor}, {A}. and {Olah}, {K}. and {Vida}, {K}. and {Wyatt}, {M}. {C}. and {Best}, {W}. {M}. {J}. and {Ciesla}, {F}. and {Csak}, {B}. and {Dupuy}, {T}. {J}. and {Handler}, {G}. and {Heng}, {K}. and {Korhonen}, {H}. and {Kovacs}, {J}. and {Kozakis}, {T}. and {Kriskovics}, {L}. and {Schmitt}, {J}. {R}. and {Szabo}, {Gy} and {Szabo}, {R}. and {Wang}, {J}. and {Goodman}, {S}. and {Hoekstra}, {A}. and {Jek}, {K}. {J}.},
urldate = {2015-11-19},
date = {2015-09-11},
keywords = {Astrophysics - Earth and Planetary Astrophysics,Astrophysics - Solar and Stellar Astrophysics},
file = {arXiv.org Snapshot:/Users/mpwd/Library/Application Support/Zotero/Profiles/fk5ookxj.default/zotero/storage/FU5W7NG4/1509.html:;arXiv\:1509.03622 PDF:/Users/mpwd/Library/Application Support/Zotero/Profiles/fk5ookxj.default/zotero/storage/GM4CN83S/Boyajian et al. - 2015 - Planet Hunters X. KIC 8462852 - Where's the Flux.pdf:application/pdf},
eprinttype = {arxiv},
eprint = {1509.03622}
}