490 citations · 3k across the 59 of their papers we have counts for
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X-ray emission from an FU Ori star in early outburst: HBC 722
Armin Liebhart, Manuel Guedel, Stephen Skinner +1
Aims: We conducted the first X-ray observations of the newly erupting FU Ori-type outburst in HBC 722 (V2493 Cyg) with the aim to characterize its X-ray behavior and near-stellar e…
Color Variability of HBC 722 in the Post-Outburst Phases
Giseon Baek, Soojong Pak, Joel D. Green +7
We carried out photometric observations for HBC 722 in SDSS r, i and z bands from 2011 April to 2013 May with a Camera for Quasars in Early uNiverse attached to the 2.1m Otto Struv…
Herschel Key Program, "Dust, Ice, and Gas In Time" (DIGIT): the origin of molecular and atomic emission in low-mass protostars in Taurus
Jeong-Eun Lee, Jinhee Lee, Seokho Lee +2
Six low-mass embedded sources (L1489, L1551-IRS5, TMR1, TMC1-A, L1527, and TMC1) in Taurus have been observed with Herschel-PACS to cover the full spectrum from 50 to 210 m as p…
Dusty Disks Around Central Stars of Planetary Nebulae
Geoffrey C. Clayton, Orsola De Marco, Jason Nordhaus +4
Only a few percent of cool, old white dwarfs (WDs) have infrared excesses interpreted as originating in small hot disks due to the infall and destruction of single asteroids that c…
Episodic Accretion in Young Stars
Marc Audard, Péter Ábrahám, Michael M. Dunham +10
In the last twenty years, the topic of episodic accretion has gained significant interest in the star formation community. It is now viewed as a common, though still poorly underst…