Flows of X-ray gas reveal the disruption of a star by a massive black hole

PS1-10jh: THE DISRUPTION OF A MAIN-SEQUENCE STAR OF NEAR-SOLAR COMPOSITION

(2014) James Guillochon et al.   ASTROPHYSICAL JOURNAL

THE TENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY: FIRST SPECTROSCOPIC DATA FROM THE SDSS-III APACHE POINT OBSERVATORY GALACTIC EVOLUTION EXPERIMENT

(2014) Christopher P. Ahn et al.   ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES

ASASSN-14ae: a tidal disruption event at 200 Mpc

(2014) T. W.-S. Holoien et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

HYDRODYNAMICAL SIMULATIONS TO DETERMINE THE FEEDING RATE OF BLACK HOLES BY THE TIDAL DISRUPTION OF STARS: THE IMPORTANCE OF THE IMPACT PARAMETER AND STELLAR STRUCTURE

(2013) James Guillochon et al.   ASTROPHYSICAL JOURNAL

An ultraviolet–optical flare from the tidal disruption of a helium-rich stellar core

(2012) S. Gezari et al.   NATURE

Observing Lense-Thirring Precession in Tidal Disruption Flares

(2012) Nicholas Stone et al.   PHYSICAL REVIEW LETTERS

Spectroscopic signatures of the tidal disruption of stars by massive black holes

(2011) Linda E. Strubbe et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

Multiband light curves of tidal disruption events

(2010) Giuseppe Lodato et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

A candidate tidal disruption event in the Galaxy cluster Abell 3571

(2009) N. Cappelluti et al.   ASTRONOMY & ASTROPHYSICS

AN ULTRA-DEEP NEAR-INFRARED SPECTRUM OF A COMPACT QUIESCENT GALAXY ATz= 2.2

(2009) Mariska Kriek et al.   ASTROPHYSICAL JOURNAL

Optical flares from the tidal disruption of stars by massive black holes

(2009) Linda E. Strubbe et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

UV/Optical Detections of Candidate Tidal Disruption Events byGALEXand CFHTLS

(2008) S. Gezari et al.   ASTROPHYSICAL JOURNAL

Stellar disruption by a supermassive black hole: is the light curve really proportional tot−5/3?

(2008) G. Lodato et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY