most citedHot Cores : Probes of High-Redshift Galaxies

22 citations · 39 across the 2 of their papers we have counts for

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astro-ph20083 cited

Using SPICA Space Telescope to characterize Exoplanets

J. R. Goicoechea, B. Swinyard, G. Tinetti +26

We present the 3.5m SPICA space telescope, a proposed Japanese-led JAXA-ESA mission scheduled for launch around 2017. The actively cooled (<5 K), single aperture telescope and mono…

astro-ph200830 cited

Molecular line profiles as diagnostics of protostellar collapse: modelling the `blue asymmetry' in inside-out infall

Y. G. Tsamis, J. M. C. Rawlings, J. A. Yates +1

The evolution of star-forming core analogues undergoing inside-out collapse is studied with a multi-point chemodynamical model which self-consistently computes the abundance distri…

astro-ph20074 cited

The SCUBA-2 "All-Sky" Survey

M. A. Thompson, S. Serjeant, T. Jenness +45

The sub-millimetre wavelength regime is perhaps the most poorly explored over large areas of the sky, despite the considerable effort that has been expended in making deep maps ove…

astro-ph200635 cited

Experimental Ti I oscillator strengths and their application to cool star analysis

R. J. Blackwell-Whitehead, H. Lundberg, G. Nave +5

We report experimental oscillator strengths for 88 Ti I transitions covering the wavelength range 465 to 3892 nm, 67 of which had no previous experimental values. Radiative lifetim…

astro-ph200522 cited

Hot Cores : Probes of High-Redshift Galaxies

C. J. Lintott, S. Viti, D. A. Williams +2

The very high rates of second generation star formation detected and inferred in high redshift objects should be accompanied by intense millimetre-wave emission from hot core molec…

astro-ph200417 cited

Molecular abundance ratios as a tracer of accelerated collapse in regions of high mass star formation?

C. J. Lintott, S. Viti, J. M. C. Rawlings +5

Recent observations suggest that the behaviour of tracer species such as N_2H+ and CS is significantly different in regions of high and low mass star formation. In the latter, N_2H…