activity
20072013
most citedMedium-separation binaries do not affect the first steps of planet formation

81 citations · 227 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2013★ 6 cited

Chemical and Physical Conditions in Molecular Cloud Core DC 000.4-19.5 (SL42) in Corona Australis

E. E. Hardegree-Ullman, J. Harju, M. Juvela +3

Chemical reactions in starless molecular clouds are heavily dependent on interactions between gas phase material and solid phase dust and ices. We have observed the abundance and d…

astro-ph.EP2012★ 41 cited

Near-UV and optical observations of the transiting exoplanet TrES-3b

Jake D. Turner, Brianna M. Smart, Kevin K. Hardegree-Ullman +23

We observed nine primary transits of the hot Jupiter TrES-3b in several optical and near-UV photometric bands from 2009 June to 2012 April in an attempt to detect its magnetic fiel…

astro-ph.CO2010★ 25 cited

LoCuSS: Shedding New Light on the Massive Lensing Cluster Abell 1689 - The View From Herschel

C. P. Haines, G. P. Smith, M. J. Pereira +5

We present wide-field Herschel/PACS observations of Abell 1689, a massive galaxy cluster at z=0.1832, from our Open Time Key Programme. We detect 39 spectroscopically confirmed 100…

astro-ph.CO2010★ 43 cited

LoCuSS: Probing Galaxy Transformation Physics with Herschel

G. P. Smith, C. P. Haines, M. J. Pereira +12

We present an early broad-brush analysis of Herschel/PACS observations of star-forming galaxies in 8 galaxy clusters drawn from our survey of 30 clusters at z~0.2. We define a comp…

astro-ph.CO2010★ 31 cited

LoCuSS: A Herschel view of obscured star formation in Abell 1835

M. J. Pereira, C. P. Haines, G. P. Smith +7

We present Herschel/PACS, MMT/Hectospec and XMM-Newton observations of Abell 1835, one of the brightest X-ray clusters on the sky, and the host of a strong cool core. Even though A…

astro-ph2007★ 81 cited

Medium-separation binaries do not affect the first steps of planet formation

I. Pascucci, D. Apai, E. E. Hardegree-Ullman +3

The first steps of planet formation are marked by the growth and crystallization of sub-micrometer-sized dust grains accompanied by dust settling toward the disk midplane. In this…