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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
2015
2015
We measure carbon radio recombination line (RRL) emission at 5.3 GHz toward four HII regions with the Green Bank Telescope (GBT… Expand
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Review
2014
Review
2014
We present optical integral field spectroscopy (IFS) observations of the Mice, a major merger between two massive (≳10^11 M_… 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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Highly Cited
2002
Highly Cited
2002
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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1998
1998
We present deep B, R and Halpha imaging of 3 dwarf galaxies: NGC3377A, NGC4286, and IC3475. Based on previous broadband imaging… Expand
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