The “Dark Side” of autophagy on the maintenance of genome stability: Does it really exist during excessive activation?

Author(s):  
Siao Muk Cheng ◽  
Min‐Chieh Shieh ◽  
Tzu‐Yu Lin ◽  
Chun Hei Antonio Cheung
2020 ◽  
Vol 21 (5) ◽  
pp. 1706 ◽  
Author(s):  
Giulia Maria Nava ◽  
Lavinia Grasso ◽  
Sarah Sertic ◽  
Achille Pellicioli ◽  
Marco Muzi Falconi ◽  
...  

In the last decade, it has become evident that RNA is frequently found in DNA. It is now well established that single embedded ribonucleoside monophosphates (rNMPs) are primarily introduced by DNA polymerases and that longer stretches of RNA can anneal to DNA, generating RNA:DNA hybrids. Among them, the most studied are R-loops, peculiar three-stranded nucleic acid structures formed upon the re-hybridization of a transcript to its template DNA. In addition, polyribonucleotide chains are synthesized to allow DNA replication priming, double-strand breaks repair, and may as well result from the direct incorporation of consecutive rNMPs by DNA polymerases. The bright side of RNA into DNA is that it contributes to regulating different physiological functions. The dark side, however, is that persistent RNA compromises genome integrity and genome stability. For these reasons, the characterization of all these structures has been under growing investigation. In this review, we discussed the origin of single and multiple ribonucleotides in the genome and in the DNA of organelles, focusing on situations where the aberrant processing of RNA:DNA hybrids may result in multiple rNMPs embedded in DNA. We concluded by providing an overview of the currently available strategies to study the presence of single and multiple ribonucleotides in DNA in vivo.


Author(s):  
P.M. Rice ◽  
MJ. Kim ◽  
R.W. Carpenter

Extrinsic gettering of Cu on near-surface dislocations in Si has been the topic of recent investigation. It was shown that the Cu precipitated hetergeneously on dislocations as Cu silicide along with voids, and also with a secondary planar precipitate of unknown composition. Here we report the results of investigations of the sense of the strain fields about the large (~100 nm) silicide precipitates, and further analysis of the small (~10-20 nm) planar precipitates.Numerous dark field images were analyzed in accordance with Ashby and Brown's criteria for determining the sense of the strain fields about precipitates. While the situation is complicated by the presence of dislocations and secondary precipitates, micrographs like those shown in Fig. 1(a) and 1(b) tend to show anomalously wide strain fields with the dark side on the side of negative g, indicating the strain fields about the silicide precipitates are vacancy in nature. This is in conflict with information reported on the η'' phase (the Cu silicide phase presumed to precipitate within the bulk) whose interstitial strain field is considered responsible for the interstitial Si atoms which cause the bounding dislocation to expand during star colony growth.


2006 ◽  
Vol 40 (12) ◽  
pp. 30
Author(s):  
BARBARA J. HOWARD
Keyword(s):  

2008 ◽  
Author(s):  
Ivelina N. Naydenova ◽  
Warren H. Jones
Keyword(s):  

2008 ◽  
Author(s):  
Amanda Poole ◽  
Julie Carswell ◽  
Rhys Lewis ◽  
Deborah Powell ◽  
Bernd Marcus

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