activity
20032022
most citedThe Spitzer Survey of the Small Magellanic Cloud: FIR Emission and Cold Gas in the SMC

216 citations · 831 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2022★ 25 cited

VERTICO III: The Kennicutt-Schmidt relation in Virgo cluster galaxies

M. J. Jiménez-Donaire, T. Brown, C. D. Wilson +19

In this VERTICO science paper we aim to study how the star formation process depends on galactic environment and gravitational interactions in the context of galaxy evolution. We e…

astro-ph.CO2010★ 96 cited

Determining dust temperatures and masses in the Herschel era: the importance of observations longward of 200 micron

K. D. Gordon, F. Galliano, S. Hony +21

The properties of the dust grains (e.g., temperature and mass) can be derived from fitting far-IR SEDs (>100 micron). Only with SPIRE on Herschel has it been possible to get high s…

astro-ph.GA2009★ 9 cited

An HST/NICMOS view of the prototypical giant HII region NGC604 in M33

Rodolfo H. Barba, Jesus Maiz Apellaniz, Enrique Perez +5

We present the first high-spatial resolution near-infrared (NIR) imaging of NGC 604, obtained with the NICMOS camera aboard the Hubble Space Telescope (HST). These NICMOS broadband…

astro-ph2008★ 46 cited

The Dust-to-Gas Ratio in the Small Magellanic Cloud Tail

K. D. Gordon, C. Bot, E. Muller +21

The Tail region of the Small Magellanic Cloud (SMC) was imaged using the MIPS instrument on the Spitzer Space Telescope as part of the SAGE-SMC Spitzer Legacy. Diffuse infrared emi…

astro-ph2007★ 55 cited

Detection of M of molecular gas in the host galaxy of the SDSS quasar J0927+2001

C. Carilli, R. Neri, R. Wang +13

We have detected emission by the CO 5-4 and 6-5 rotational transitions at from the host galaxy of the SDSS quasar J0927+2001 using the Plateau de Bure interf…

astro-ph2007★ 28 cited

Self-consistent massive disks in triaxial dark matter halos

Jeremy Bailin, Josh D. Simon, Alberto D. Bolatto +2

Galactic disks in triaxial dark matter halos become deformed by the elliptical potential in the plane of the disk in such a way as to counteract the halo ellipticity. We develop a…