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most citedThe imprint of exoplanet formation history on observable present-day spectra of hot Jupiters

391 citations · 4.6k across the 83 of their papers we have counts for

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Showing 2010Show all

6 papers · 1 filter

astro-ph.SR2010★ 46 cited

Fundamental Vibrational Transition of CO during the Outburst of EX Lupi in 2008

M. Goto, Zs. Regály, C. P. Dullemond +16

We report monitoring observations of the T Tauri star EX Lupi during its outburst in 2008 in the CO fundamental band at 4.6-5.0 um. The observations were carried out at the VLT and…

astro-ph.SR2010★ 28 cited

Detectability of giant planets in protoplanetary disks by CO emission lines

Zs. Regaly, Zs. Sandor, C. P. Dullemond +1

In this paper we intend to provide an indirect method to detect Jovian planets by studying near infrared emission spectra originating in the protoplanetary disks around T Tauri sta…

astro-ph.SR2010★ 12 cited

Mid - infrared interferometry of massive young stellar objects II Evidence for a circumstellar disk surrounding the Kleinmann - Wright object

R. Follert, H. Linz, B. Stecklum +5

The formation scenario for massive stars is still under discussion. To further constrain current theories, it is vital to spatially resolve the structures from which material accre…

astro-ph.SR2010★ 95 cited

On the origin of [NeII] 12.81 micron emission from pre-main sequence stars: Disks, jets, and accretion

M. Guedel, F. Lahuis, K. R. Briggs +6

(Abridged) We have conducted a study of [NeII] line emission based on a sample of 92 pre-main sequence stars mostly belonging to the infrared Class II, including 13 accreting trans…

astro-ph.EP2010★ 38 cited

Variable accretion as a mechanism for brightness variations in T Tau S

Roy van Boekel, Attila Juhasz, Thomas Henning +5

(Note: this is a shortened version of the original A&A-style structured abstract). The physical nature of the strong photometric variability of T Tau Sa, the more massive member of…

astro-ph.SR2010★ 30 cited

HD 95881: A gas rich to gas poor transition disk?

A. P. Verhoeff, M. Min, B. Acke +8

Context. Based on the far infrared excess the Herbig class of stars is divided into a group with flaring circumstellar disks (group I) and a group with flat circumstellar disks (gr…