A Kpc-scale Radio Polarization Study of PG BL Lacs with the uGMRT
| Autor: | Baghel, Janhavi, Kharb, P., Hovatta, T., Gulati, S., Lindfors, E., S, Silpa |
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| Rok vydání: | 2023 |
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| Druh dokumentu: | Working Paper |
| Popis: | We present here uGMRT band 4 (~650MHz) polarization images of 8 BL~Lac objects belonging to the Palomar-Green (PG) `blazar' sample. A large fraction of the sources (~63%) reveal core-halo radio structures with most of the polarization detected in the inner core-jet regions. PG1101+385 and PG2254+075 exhibit a `spine-sheath structure' in polarization. The core-halo and `spine-sheath' structures are consistent with the Unified Scheme suggestion that BL~Lacs are the pole-on beamed counterparts of Fanaroff-Riley (FR) type I radio galaxies. PG1418+546 and PG0851+203 (OJ287) show the presence of terminal hotspots similar to FR type II radio galaxies. They were also found to be low-spectrally peaked BL Lacs, supportive of the `blazar envelope' scenario for BL~Lacs and quasars. Fractional polarization ranges from 1-13% in the cores and 2-26% in the inner jets/lobes of the sample BL Lacs. Compared to the varied radio morphology of quasars from the PG `blazar' sample, the BL~Lacs appear to be less diverse. A comparison of the inferred core magnetic (B-) field structures on arcsec- (kpc-) scales w.r.t. the Very Long Baseline Interferometry (VLBI) jet direction does not reveal any preferred orientation, suggesting that if large-scale ordered B-fields exist, they do so on scales smaller than probed by the current observations. However, the presence of polarized emission on arcsec-scales suggests that any mixing of thermal plasma with the synchrotron emitting plasma is insufficient to fully depolarize the emission via the internal depolarization process. Comment: 17 pages; 12 figures; MNRAS accepted |
| Databáze: | arXiv |
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