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NGC-III protein, mouse

 
National Institutes of Health

Papers overview

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2018
2018
The presence and properties of compact radio sources embedded in massive star-forming regions can reveal important physical… Expand
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2016
2016
We measured Surface Brightness FluctuaIons (SBF) in three galaxies, ESO137-G006, NGC 3309, and NGC 5128, using the GeMS… Expand
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2015
2015
We measure carbon radio recombination line (RRL) emission at 5.3 GHz toward four H ii regions with the Green Bank Telescope to… Expand
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2014
2014
The effect of thermal-oxidative treatment on the structure and conductive properties of nanosized globular carbon (NGC) P 234 was… Expand
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2011
2011
We present an analysis of the Suzaku observations of the prototype wind-blown bubble NGC 6888 which is based both on use of… Expand
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Highly Cited
2006
Highly Cited
2006
Motivated by the recent discovery of 30 new millisecond pulsars in Terzan 5, made using the Green Bank Telescope's S-band… Expand
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2003
2003
The results from an X-ray spectroscopic study of the giant elliptical galaxy NGC 5044 in the center of a galaxy group are… Expand
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2002
2002
The sparse stellar ensemble NGC 6994 = M 73 has recently been discussed as a possible remnant of an old open cluster. In order to… Expand
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2000
2000
Communication networks go through frequent upgrades, whereby access point (AP) devices that serve network client devices are… Expand
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1999
1999
We present deep B-band, R-band, and Hα imaging of three dwarf galaxies: NGC 3377A, NGC 4286, and IC 3475. Based on previous… Expand
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