| Literature DB >> 30571776 |
Michele C Paula1,2, Kamylla B Michelutti1,3, Aylson D M M Eulalio1,2, Raul C Piva4, Claudia A L Cardoso3,4, William F Antonialli-Junior1,2,3.
Abstract
Most flies of forensic importance are in two superfamilies, the Muscoidea and the Oestroidea, with similar life stages including the puparium. Upon completion of metamorphosis the adult fly emerges from the puparium, leaving behind an exuvia that is of potential significance in forensic investigation. The empty puparium is a durable piece of entomological evidence lasting several years. Through the study of chemical compounds, specifically the hydrocarbons of these puparia, it is possible to identify the species, in addition to how long they have been exposed to weathering and for this reason, these parameters can assist forensic entomologists in estimating long-term postmortem interval (minPMI). In corpses that take a relatively longer time to decompose, insects may use the same corpses for several oviposition cycles. Therefore, the aim of this study was to develop a new method to determine the PMI based on chemical compounds of the puparia from different oviposition cycles of the fly Chrysomya megacephala. The chemical composition of 50 puparia from different cycles of oviposition were evaluated by Gas Chromatography-Mass Spectrometry (GC-MS). In total, 60 compounds were identified ranging from C18 to C34, 38 of those were common to all generations. Our results demonstrate that chemical profiles can be used to differentiate puparia collected from successive cycles, and therefore valuable in the estimation of minPMI.Entities:
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Year: 2018 PMID: 30571776 PMCID: PMC6301778 DOI: 10.1371/journal.pone.0209776
Source DB: PubMed Journal: PLoS One ISSN: 1932-6203 Impact factor: 3.240
Relative proportions of cuticular hydrocarbons present in empty puparia of three generations of the blow fly Chrysomya megacephala.
| Peak | RT (min) | Compound | ECL | 1st Generation (F1) | 2nd Generation (F2) | 3rd Generation |
|---|---|---|---|---|---|---|
| Relative Abundance (% ± Standard Deviation) | ||||||
| 1 | 13.255 | 3- MeC18 | 1875 | 1.90±0.27 | 2.04±1.45 | 2.42±0.75 |
| 2 | 15.769 | 2-MeC19 | 1969 | 10.43±5.19 | 0.58±0.42 | 0.28±0.06 |
| 3 | 15.909 | 3-MeC19 | 1975 | ND | 0.42±0.77 | 0.19±0.07 |
| 4 | 16.546 | C20 | 2000 | ND | 0.58±0.06 | 0.11±0.07 |
| 5 | 19.283 | C21 | 2100 | ND | 0.28±0.30 | 0.21±0.04 |
| 6 | 20.180 | 9-MeC21 | 2131 | ND | 0.41±0.81 | 0.13±0.09 |
| 7 | 20.781 | 5-MeC21 | 2153 | 37.75±12.64 | ND | ND |
| 8 | 20.872 | 4-MeC21 | 2156 | 12.56±2.33 | ND | ND |
| 9 | 22.148 | C22 | 2200 | ND | 0.52±10 | 0.18±0.12 |
| 10 | 24.163 | C23:1 | 2278 | ND | 0.16±0.38 | ND |
| 11 | 24.769 | C23 | 2300 | 0.12±0.05 | 1.55±1.02 | 0.52±0.24 |
| 12 | 27.390 | C24 | 2400 | ND | 1.19±0.71 | 0.24±0.31 |
| 13 | 29.512 | C25:1 | 2484 | 1.07±3.03 | ND | ND |
| 14 | 29.929 | C25 | 2500 | 0.40±0.11 | 1.26±0.66 | 1.24±0.34 |
| 15 | 31.270 | 7-MeC25 | 2554 | 0.24±0.07 | 0.34±0.27 | 1.11±1.89 |
| 16 | 31.484 | 2-MeC25 | 2563 | ND | 0.95±1.86 | 0.15±0.12 |
| 17 | 32.398 | C26 | 2600 | 0.19±0.03 | 0.47±0.24 | 0.34±0.28 |
| 18 | 33.258 | 13-MeC26 | 2641 | 0.11±0.03 | 0.34±0.55 | ND |
| 19 | 33.897 | 3-MeC26 | 2672 | 0.11±0.02 | 0.69±1.07 | 0.12±0.04 |
| 20 | 34.354 | C27:1 | 2693 | ND | 0.96±1.56 | ND |
| 21 | 34.614 | C27 | 2700 | 3.01±1.31 | 7.41±1.20 | 8.61±1.47 |
| 22 | 35.555 | 7-MeC27 | 2741 | ND | 7.67±10.66 | 0.38±0.40 |
| 23 | 36.235 | 2-MeC27 | 2767 | 0.43±0.82 | 0.81±1.16 | 0.21±0.07 |
| 24 | 36.490 | C28:1 | 2777 | 0.81±0.41 | 1.39±0.40 | 2.54±0.51 |
| 25 | 37.093 | C28 | 2800 | 0.41±0.13 | 0.74±0.25 | 0.76±0.18 |
| 26 | 37.828 | 14-MeC28 | 2833 | 0.35±0.22 | 5.20±1.97 | 3.00±0.42 |
| 27 | 38.009 | x-MeC28
| 2841 | 0.03±0.03 | 0.75±1.56 | 0.03±0.07 |
| 28 | 38.511 | 2-MeC28 | 2863 | 2.60±1.14 | 8.30±1.46 | 9.59±1.06 |
| 29 | 38.966 | 4,12-DiMeC28 | 2884 | ND | 1.99±2.96 | ND |
| 30 | 39.183 | C29:1 | 2893 | 0.33±0.13 | 0.71±0.4 | 1.77±0.58 |
| 31 | 39.347 | C29 | 2900 | 5.48±2.11 | 12.56±4.81 | 16.97±3.21 |
| 32 | 40.001 | 13-MeC29 | 2931 | 0.92±0.38 | 5.33±4.12 | 4.10±0.61 |
| 33 | 40.123 | 7-MeC29 | 2937 | 0.11±0.03 | 0.26±0.24 | 0.04±0.13 |
| 34 | 40.233 | 9-MeC29 | 2942 | 0.21±0.10 | 0.17±0.24 | 0.68±0.12 |
| 35 | 40.437 | 5-MeC29 | 2951 | 0.33±0.16 | 0.50±0.12 | 0.86±0.15 |
| 36 | 40.597 | 11,15-;17,15-;9,17-;9,19-DiMeC29 | 2958 | 0.12±0.03 | 0.53±0.86 | 0.13±0.09 |
| 37 | 40.703 | 11,19-DiMeC29 | 2963 | 0.11±0.06 | 0.14±0.08 | 0.14±0.14 |
| 38 | 40.943 | 7,17-DiMeC29 | 2974 | 0.70±0.32 | 1.11±0.51 | 2.84±0.71 |
| 39 | 41.077 | 5,13-DiMeC29 | 2981 | 0.14±0.04 | 0.44±0.83 | 0.19±0.10 |
| 40 | 41.500 | C30 | 3000 | 0.26±0.09 | 0.23±0.11 | 0.40±0.10 |
| 41 | 41.685 | 3,9-;3,11-;3,13-DiMeC30 | 3009 | 0.13±0.10 | 0.13±0.07 | 0.27±0.17 |
| 42 | 42.127 | 15-;14-MeC30 | 3030 | 0.53±0.26 | 1.13±0.31 | 1.45±0.34 |
| 43 | 42.819 | 2-MeC30 | 3063 | 1.39±0.78 | 1.98±0.71 | 2.68±0.42 |
| 44 | 43.427 | C31:1 | 3092 | 0.52±0.27 | 0.63±0.44 | 1.69±0.37 |
| 45 | 43.602 | C31 | 3100 | 1.41±0.39 | 1.77±0.94 | 3.05±1.70 |
| 46 | 44.205 | 15-;13-MeC31 | 3130 | 4.93±2.57 | 12.46±5.27 | 17.34±1.53 |
| 47 | 44.432 | 7-MeC31 | 3141 | 0.35±0.20 | 0.7±0.34 | 1.46±0.34 |
| 48 | 44.724 | 13,17-DiMeC31 | 3155 | 1.59±0.73 | 4.3±1.68 | 4.88±0.78 |
| 49 | 44.999 | 9,17-;9,19-;9,21-DiMeC31 | 3169 | 0.17±0.08 | 0.14±0.08 | 0.16±0.20 |
| 50 | 46.207 | 11-MeC32 | 3229 | 0.68±0.37 | 0.69±0.31 | 0.86±0.15 |
| 51 | 46.399 | 10-;12-;13-;14-MeC32 | 3238 | 0.3±0.10 | 0.13±0.11 | ND |
| 52 | 46.701 | 12,16 -DiMeC32 | 3254 | 0.24±0.17 | 0.12±0.16 | 0.23±0.18 |
| 53 | 46.872 | 2-MeC32 | 3262 | 0.25±0.22 | ND | ND |
| 54 | 47.437 | C33:1 | 3291 | 0.2±0.17 | ND | ND |
| 55 | 47.605 | C33 | 3200 | 0.13±0.08 | ND | ND |
| 56 | 48.237 | 13-MeC33 | 3332 | 2.62±1.11 | 2.25±1.2 | 3.56±0.91 |
| 57 | 48.628 | 13, 17-DiMeC33 | 3353 | 1.13±0.76 | 1.1±0.65 | 1.06±0.34 |
| 58 | 48.937 | 11,17,21-;11,17,23-TriMeC33 | 3370 | 0.004±0.01 | 0.19±0.16 | ND |
| 59 | 49.271 | 9,13,17-;9,15,19-;9,15,21;9,15,23-TriMeC33 | 3386 | 0.17±0.11 | ND | ND |
| 60 | 51.331 | C34:1 | 3492 | 0.17±0.18 | ND | ND |
* = Compounds present in all generations; ND = Not detected; ECL = equivalent chain length; RT = Retention time.
Fig 1Representative profiles of compound present in empty puparia Chrysomya megacephala.
(a) = GC chromatograms of 1st; (b) = GC chromatograms of 2nd and (c) = GC chromatograms of 3rd generation of the blow fly Chrysomya megacephala. Numbers refer to the substances listed in Table 1.
Fig 2Bar graphic of compound classes present in empty puparia Chrysomya megacephala.
(a) = Mean percentages of compound classes; (b) = Number of compounds present in empty puparia of three different generations of the blow fly Chrysomya megacephala.
Fig 3Dispersion diagram showing the results assessed by GC-MS of the specie Chrysomya megacephala.
Differentiation of the cuticular chemical profile in empty puparia of three different generations of the blow fly Chrysomya megacephala.