Persistent organic pollutants (POPs)
have received significant
and ongoing attention. To establish favorable regulatory policies,
it is vital to investigate the occurrence, source, and budgets of
POPs worldwide. POPs including phthalic acid esters (PAEs), organophosphate
esters (OPEs), brominated flame retardants (BFRs), and highly chlorinated
flame retardants (HFRs) have not yet been examined in the Eastern
Indian Ocean (EIO). In this study, the distribution of POPs has been
investigated from surface sediments with the depth of 4369–5742
m in the Central Indian Ocean Basin (CIOB) and Wharton Basin (WB)
of EIO. The average (±SD) concentrations of ∑11PAEs, ∑11OPEs, ∑4 BFRs, and ∑5HFRs were 1202.0 ± 274.36 ng g–1 dw,
15.3 ± 7.23 ng g–1 dw, 327.6 ± 211.74
pg g–1 dw, and 7.9 ± 7.45 pg g–1 dw, respectively. The high abundance of low-molecular-weight (LMW)
PAEs, chlorinated OPEs, LMW BDEs, and anti-Dechlorane Plus indicated
the pollution characteristics in the EIO. Correlation analysis demonstrated
that LMW compounds may be derived from the high-molecular-weight compounds.
The monsoon circulation, currents, and Antarctic Bottom Water may
be the main drivers. POP accumulation rate, depositional flux, and
mass inventory in the Indian Ocean were also estimated.