activity
20032009
most citedWFCAM, Spitzer-IRAC and SCUBA observations of the massive star forming region DR21/W75: I. The collimated molecular jets

191 citations · 280 across the 6 of their papers we have counts for

collaborators

9 papers

astro-ph.EP2009

MRO/CRISM Retrieval of Surface Lambert Albedos for Multispectral Mapping of Mars with DISORT-based Rad. Transfer Modeling: Phase 1 - Using Historical Climatology for Temperatures, Aerosol Opacities, & Atmo. Pressures

P. C. McGuire, M. J. Wolff, M. D. Smith +22

We discuss the DISORT-based radiative transfer pipeline ('CRISM_LambertAlb') for atmospheric and thermal correction of MRO/CRISM data acquired in multispectral mapping mode (~200 m…

astro-ph2008

Protostellar fountains do shape the regional core mass function?

J. Z. Li, M. D. Smith, M. Huang +1

Paper withdrawn, sorry for any inconvenience raised!

astro-ph200833 cited

Near-infrared, IFU spectroscopy unravels the bow-shock HH99B

T. Giannini, L. Calzoletti, B. Nisini +3

We aim to characterise the morphology and the physical parameters governing the shock physics of the Herbig-Haro object HH99B. We have obtained SINFONI-SPIFFI IFU spectroscopy betw…

astro-ph200733 cited

VLT / Infrared Integral Field Spectrometer Observations of Molecular Hydrogen Lines in the Knots in the Planetary Nebula NGC 7293 (the Helix Nebula)

M. Matsuura, A. K. Speck, M. D. Smith +6

Knots are commonly found in nearby planetary nebulae (PNe) and star forming regions. Within PNe, knots are often found to be associated with the brightest parts of the nebulae and…

astro-ph2006191 cited

WFCAM, Spitzer-IRAC and SCUBA observations of the massive star forming region DR21/W75: I. The collimated molecular jets

C. J. Davis, M. S. N. Kumar, G. Sandell +3

We present wide-field near-infrared images of the DR21/W75 high-mass star forming region, obtained with the Wide Field Camera, WFCAM, on the United Kingdom Infrared Telescope. Broa…

astro-ph200623 cited

An Outbursting Protostar of the FU~Orionis type in the Cygnus OB7 Molecular Cloud

T. A. Movsessian, T. Khanzadyan, C. Aspin +5

Context: To follow the early evolution of stars we need to understand how young stars accrete and eject mass. It is generally assumed that the FU Orionis phenomenon is related to t…