Clinical surveillance for human astrovirus in Monastir region, Tunisia

Abir Monastiri1, Mahjoub Aouni2, Susana Guix3

  • 1Laboratory of Contagious Diseases and Biologically Active Substances, LR99ES27, Faculty of Pharmacy, University of Monastir, Avicenne Street 5000, Monastir, Tunisia. abirmonastiri@gmail.com.

BMC Public Health
|January 23, 2016
PubMed

Insights

Human astrovirus (HAstV) prevalence in Tunisian children with gastroenteritis is low (4%). Phylogenetic analysis revealed HAstV-3c strains circulating in 2010, suggesting potential emergence, alongside earlier HAstV-3a strains.

Area of Science:

  • Virology
  • Pediatric Gastroenterology
  • Public Health

Background:

  • Astroviruses (AstVs) are a common cause of gastroenteritis in young children.
  • Monitoring AstV circulation is crucial for understanding pediatric infectious diseases.

Purpose of the Study:

  • To determine the prevalence of human astrovirus (HAstV) in children with acute gastroenteritis in Monastir, Tunisia.
  • To characterize circulating HAstV strains and assess their infectivity.
  • To conduct phylogenetic analysis of isolated HAstV strains.

Main Methods:

  • Stool samples were collected from 50 children under five years old.
  • Reverse transcription-polymerase chain reaction (RT-PCR) was used for viral detection.
  • Sequencing, phylogenetic analysis, and cell culture (CaCO-2) were employed for characterization and infectivity assessment.

Main Results:

  • A low prevalence of astrovirus (4%) was observed in the study population.
  • The two positive samples were identified as HAstV type 3.
  • Phylogenetic analysis indicated two distinct HAstV-3 lineages: HAstV-3a (2004 strains) and HAstV-3c (2010 strains).
  • Infectious viral particles were confirmed in positive samples cultured on CaCO-2 cells.

Conclusions:

  • The study confirms a low prevalence of astrovirus in children with gastroenteritis in Monastir, Tunisia.
  • Circulating HAstV-3c strains identified in 2010 may represent an emerging lineage.
  • The findings highlight the co-circulation of different HAstV-3 lineages (3a and 3c) over time in the region.
Abstract