most citedPeriodic accretion from a circumbinary disk in the young binary UZ Tau E

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astro-ph20081 cited

Fundamental Properties of Low-Mass Stars and Brown Dwarfs

Michael C. Liu, Keivan G. Stassun, France Allard +7

Precise measurements of the fundamental properties of low-mass stars and brown dwarfs are key to understanding the physics underlying their formation and evolution. While there has…

astro-ph200832 cited

The Pre-Main-Sequence Eclipsing Binary ASAS J052821+0338.5

H. C. Stempels, L. Hebb, K. G. Stassun +4

In this paper we present the first results of a detailed spectroscopic and photometric analysis of the V = 11.7m eclipsing binary ASAS J052821+0338.5. With the FIES spectrograph at…

astro-ph200727 cited

Detection of strong activity in the eclipsing binary brown dwarf 2MASSJ05352184-0546085 - A possible explanation for the temperature reversal

A. Reiners, A. Seifahrt, K. G. Stassun +2

We show high resolution spectra of the eclipsing brown dwarf binary 2MASSJ05352184-0546085 taken at the two opposite radial velocity maxima. Comparisons of the TiO bands to model a…

astro-ph200739 cited

Discovery of Par 1802 as a Low-Mass, Pre-Main-Sequence Eclipsing Binary in the Orion Star-Forming Region

P. A. Cargile, K. G. Stassun, R. D. Mathieu

We report the discovery of a pre-main-sequence, low-mass, double-lined, spectroscopic, eclipsing binary in the Orion star-forming region. We present our observations including radi…

astro-ph200750 cited

The Monitor project: JW 380 -- a 0.26, 0.15 Msol pre main sequence eclipsing binary in the Orion Nebula Cluster

Jonathan Irwin, Suzanne Aigrain, Simon Hodgkin +14

We report the discovery of a low-mass (0.26 +/- 0.02, 0.15 +/- 0.01 Msol) pre-main-sequence eclipsing binary with a 5.3 day orbital period. JW 380 was detected as part of a high-ca…

astro-ph200783 cited

Periodic accretion from a circumbinary disk in the young binary UZ Tau E

Eric L. N. Jensen, Saurav Dhital, Keivan G. Stassun +6

Close pre-main-sequence binary stars are expected to clear central holes in their protoplanetary disks, but the extent to which material can flow from the circumbinary disk across…