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19992026
most citedThe Magnetic Fields of Classical T Tauri Stars

401 citations · 6.1k across the 115 of their papers we have counts for

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Showing 2010Show all

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astro-ph.SR2010★ 71 cited

The search for magnetic fields in mercury-manganese stars

V. Makaganiuk, O. Kochukhov, N. Piskunov +7

We performed a highly sensitive search for magnetic fields on a large set of HgMn stars. With the aid of a new polarimeter attached to the HARPS spectrometer at the ESO 3.6m-telesc…

astro-ph.IM2010★ 5 cited

The HARPS polarimeter

Frans Snik, Oleg Kochukhov, Nikolai Piskunov +8

We recently commissioned the polarimetric upgrade of the HARPS spectrograph at ESO's 3.6-m telescope at La Silla, Chile. The HARPS polarimeter is capable of full Stokes spectropola…

astro-ph.SR2010★ 33 cited

The Light Curve of the Weakly-Accreting T Tauri Binary KH 15D from 2005-10: Insights into the Nature of its Protoplanetary Disk

William Herbst, Katherine LeDuc, Catrina M. Hamilton +4

Photometry of the unique pre-main sequence binary system KH 15D is presented, spanning the years 2005-2010. This system has exhibited photometric variations and eclipses over the l…

astro-ph.EP2010★ 43 cited

NICMOS Observations of the Transiting Hot Jupiter XO-1b

Christopher J. Burke, P. R. McCullough, E. Bergeron +6

We refine the physical parameters of the transiting hot Jupiter planet XO-1b and its stellar host XO-1 using HST NICMOS observations. XO-1b has a radius Rp=1.21+/-0.03 RJup, and XO…

astro-ph.SR2010★ 9 cited

Gas Absorption in the KH 15D System: Further Evidence for Dust Settling in the Circumbinary Disk

S. M. Lawler, W. Herbst, S. Redfield +5

Na I D lines in the spectrum of the young binary KH 15D have been analyzed in detail. We find an excess absorption component that may be attributed to foreground interstellar absor…

astro-ph.EP2010★ 52 cited

Thermal Emission and Tidal Heating of the Heavy and Eccentric Planet XO-3b

Pavel Machalek, Tom Greene, Peter R. McCullough +5

We determined the flux ratios of the heavy and eccentric planet XO-3b to its parent star in the four IRAC bands of the Spitzer Space Telescope: 0.101% +- 0.004% at 3.6 micron; 0.14…