Results 171 to 180 of about 1,920 (202)
Dominant Negative Mutants of the Murine Cytomegalovirus M53 Gene Block Nuclear Egress and Inhibit Capsid Maturation [PDF]
The alphaherpesvirus proteins UL31 and UL34 and their homologues in other herpesvirus subfamilies cooperate at the nuclear membrane in the export of nascent herpesvirus capsids.
Zsolt Ruzsics +2 more
exaly +4 more sources
We report CCD V and I time series photometry of the globular cluster NGC 5024 (M53). The technique of difference image analysis has been used which enables photometric precisions better than 10 mmag for stars brighter than V˜ 18.5 mag even in the crowded
A Arellano Ferro +2 more
exaly +4 more sources
Internal Rotation in the Globular Cluster M53
This record is for a(n) offprint of an article published in The Astrophysical Journal on 2017-05-31; the version of record is available at https://doi.org/10.3847/1538-4357/aa7070.We present an analysis of the internal bulk rotation in the metal-poor ...
Owen M Boberg +2 more
exaly +2 more sources
Light Element Abundances and Multiple Populations in M53 [PDF]
Abstract We present results from a study of 94 red giant stars in the globular cluster M53. We use low-resolution spectra to measure the strength of CN and CH features at ∼3800 and 4300 Å, respectively. The strengths of these features are used to classify stars into a CN-enhanced and CN-normal population and to measure C and N abundances
Jeffrey M Gerber +2 more
exaly +3 more sources
Study of globular cluster M53: new variables, distance, metallicity [PDF]
We study the variable star content of the globular cluster M53 to compute the physical parameters of the constituting stars and the distance of the cluster. Covering two adjacent seasons in 2007 and 2008, new photometric data are gathered for 3048 objects in the field of M53.
I Dekany
exaly +3 more sources
New SX Phoenicis Stars in the Globular Cluster M53
31 pages with 7 figures, accepted by the Astronomical Journal (scheduled June 2003)
Young-Beom Jeon +2 more
exaly +3 more sources
RELATIVE AGE DIFFERENCE BETWEEN THE METAL-POOR GLOBULAR CLUSTERS M53 AND M92
CCD photometric observations of the globular cluster (GC), M53 (NGC 5024), are performed using the 1.8 m telescope at the Bohyunsan Optical Astronomy Observatory in Korea on the same nights (2002 April and 2003 May) as the observations of the GC M92 (NGC 6341) reported by Cho and Lee using the same instrumental setup.
Hyun-Il Sung, Sang-Gak Lee
exaly +3 more sources
Radio sources near the globular clusters M13 and M53
S j jr Goldstein, C M Wade
exaly +2 more sources

