Showing 1–18 of 18 results
/ Date/ Name
Sep 17, 2015The 2010 Eruption of the Recurrent Nova U Scorpii: The Multi-Wavelength Light CurveAug 14, 2009Discovery of a Second Nova Eruption of V2487 OphiuchiMay 1, 2014Identifying and Quantifying Recurrent Novae Masquerading as Classical NovaeJan 30, 2012The Progenitor of the Type Ia Supernova that created SNR 0519-69.0 in the Large Magellanic CloudMar 30, 2016Non-Detection of Nova Shells Around Asynchronous PolarsJan 3, 2015Investigation of the Progenitors of the Type Ia Supernovae Associated With the LMC Supernova Remnants 0505-67.9 and 0509-68.7May 1, 2014The Diffuse Source at the Center of LMC SNR 0509-67.5 is a Background Galaxy at z = 0.031May 2, 2019Precise Measures of Orbital Period, Before and After Nova Eruption for QZ AurigaeSep 23, 2009The Behavior of Novae Light Curves Before EruptionJan 10, 2012The center of the Type Ia supernova remnant SNR 0509-67.5 is empty of any ex-companion star to M_V=+8.4Mar 31, 2017Nova Scorpius 1437 A.D. is now a dwarf nova, age-dated by its proper motionMar 30, 2015HST Images Flash Ionization of Old Ejecta by the 2011 Eruption of Recurrent Nova T PyxidisAug 4, 2011Eclipses During the 2010 Eruption of the Recurrent Nova U ScorpiiJan 11, 2022Discovery of Extreme, Roughly-Daily Superflares on the Recurrent Nova V2487 OphFeb 22, 2017A Hubble Space Telescope survey for novae in M87. III. Are novae good standard candles 15 days after maximum brightness?Aug 23, 2011NSV 11154 Is a New R Coronae Borealis StarJun 4, 2009The Nova Shell and Evolution of the Recurrent Nova T PyxidisApr 16, 2010Discovery of the 2010 Eruption and the Pre-Eruption Light Curve for Recurrent Nova U Scorpii