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VLA H53α Radio Recombination Line Observations of the Ultraluminous Infrared Galaxy Arp 220

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C. A. Rodríguez-Rico1,2, W. M. Goss2, F. Viallefond3, J.-H. Zhao4, Y. Gómez1 and K. R. Anantharamaiah5

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[1]

Unveiling Extragalactic Star Formation Using Radio Recombination Lines: An Expanded Very Large Array Pilot Study with NGC 253

Amanda A. Kepley et al.  The Astrophysical Journal Letters 2011  739 L24
IOPscience 
[2]

Evaluating the Calorimeter Model with Broadband, Continuous Spectra of Starburst Galaxies Observed with the Allen Telescope Array

Peter K. G. Williams and Geoffrey C. Bower  The Astrophysical Journal 2010  710 1462
IOPscience 
[3]

Submillimeter Array Imaging of the CO(3-2) Line and 860 μm Continuum of Arp 220: Tracing the Spatial Distribution of Luminosity

Kazushi Sakamoto et al.  The Astrophysical Journal 2008  684 957
IOPscience 
[4]

VLA H53α Observations of the Central Region of the Super Star Cluster Galaxy NGC 5253

C. A. Rodríguez-Rico et al.  The Astrophysical Journal 2007  670 295
IOPscience 
[5]

The Radio Spectra of the Compact Sources in Arp 220: A Mixed Population of Supernovae and Supernova Remnants

Rodrigo Parra et al.  The Astrophysical Journal 2007  659 314
IOPscience 
[6]

A New Water Vapor Megamaser

José Cernicharo et al  The Astrophysical Journal Letters 2006  646 L49
IOPscience 
[7]

VLBI Images of 49 Radio Supernovae in Arp 220

Colin J. Lonsdale et al.  The Astrophysical Journal 2006  647 185
IOPscience 
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