2024A&A...683A..70H

Query : 2024A&A...683A..70H

2024A&A...683A..70H - Astronomy and Astrophysics, volume 683A70 (2024/3-1)

TeV flaring activity of the AGN PKS 0625-354 in November 2018.

HESS COLLABORATION, AHARONIAN F., AIT BENKHALI F., ASCHERSLEBEN J., ASHKAR H., BACKES M., BAKTASH A., BARBOSA MARTINS V., BARNARD J., BATZOFIN R., BECHERINI Y., BERGE D., BERNLOHR K., BI B., BOTTCHER M., BOISSON C., BOLMONT J., DE BONY DE LAVERGNE M., BOROWSKA J., BRADASCIO F., BREUHAUS M., BROSE R., BROWN A., BRUN F., BRUNO B., BULIK T., BURGER-SCHEIDLIN C., BYLUND T., CAROFF S., CASANOVA S., CECIL R., CELIC J., CERRUTI M., CHAND T., CHANDRA S., CHEN A., CHIBUEZE J., CHIBUEZE O., COTTER G., DAMASCENE MBARUBUCYEYE J., DAVIDS I.D., DJUVSLAND J., DMYTRIIEV A., DOROSHENKO V., EGBERTS K., EINECKE S., ERNENWEIN J.-P., FONTAINE G., FUSSLING M., FUNK S., GABICI S., GHAFOURIZADEH S., GIAVITTO G., GLAWION D., GLICENSTEIN J.F., GLOMBITZA J., GOSWAMI P., GROLLERON G., HAERER L., HINTON J.A., HOLCH T.L., HOLLER M., HORNS D., JAMROZY M., JANKOWSKY F., JOSHI V., JUNG-RICHARDT I., KASAI E., KATARZYNSKI K., KHATOON R., KHELIFI B., KLUZNIAK W., KOMIN N., KOSACK K., KOSTUNIN D., LANG R.G., LE STUM S., LEITL F., LEMIERE A., LENAIN J.-P., LEUSCHNER F., LUASHVILI A., MACKEY J., MARX R., MEHTA A., MEYER M., MITCHELL A., MODERSKI R., MONTANARI A., MOULIN E., DE NAUROIS M., NIEMIEC J., O'BRIEN P., OHM S., OLIVERA-NIETO L., DE ONA WILHELMI E., OSTROWSKI M., PANNY S., PARSONS R.D., PITA S., PROKHOROV D.A., PUHLHOFER G., PUNCH M., QUIRRENBACH A., REICHHERZER P., REIMER A., REIMER O., REN H., RIEGER F., RUDAK B., SAHAKIAN V., SALZMANN H., SANCHEZ D.A., SASAKI M., SCHUSSLER F., SCHUTTE H.M., SHAPOPI J.N.S., SOL H., SPECOVIUS A., SPENCER S., STAWARZ L., STEENKAMP R., STEINMASSL S., STREIL K., SUSHCH I., SUZUKI H., TAKAHASHI T., TANAKA T., VAN ELDIK C., VECCHI M., VEH J., VENTER C., WAGNER S.J., WIERZCHOLSKA A., ZACHARIAS M., ZARGARYAN D., ZDZIARSKI A.A., ZECH A., ZOUARI S. and ZYWUCKA N.

Abstract (from CDS):

Most γ-ray detected active galactic nuclei are blazars with one of their relativistic jets pointing towards the Earth. Only a few objects belong to the class of radio galaxies or misaligned blazars. Here, we investigate the nature of the object PKS 0625-354, its γ-ray flux and spectral variability and its broad-band spectral emission with observations from H.E.S.S., Fermi-LAT, Swift-XRT, and UVOT taken in November 2018. The H.E.S.S. light curve above 200 GeV shows an outburst in the first night of observations followed by a declining flux with a halving time scale of 5.9 h. The γγ-opacity constrains the upper limit of the angle between the jet and the line of sight to ∼10°. The broad-band spectral energy distribution shows two humps and can be well fitted with a single-zone synchrotron self Compton emission model. We conclude that PKS 0625-354, as an object showing clear features of both blazars and radio galaxies, can be classified as an intermediate active galactic nuclei. Multi-wavelength studies of such intermediate objects exhibiting features of both blazars and radio galaxies are sparse but crucial for the understanding of the broad-band emission of γ-ray detected active galactic nuclei in general.

Abstract Copyright: © The Authors 2024

Journal keyword(s): galaxies: active - galaxies: individual: PKS 0625-354 - galaxies: jets - gamma rays: galaxies

Simbad objects: 8

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Number of rows : 8
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 IC 310 AGN 03 16 42.9787569912 +41 19 29.615579544   14.3       ~ 311 2
2 NGC 1275 Bla 03 19 48.1599902040 +41 30 42.108850836   13.10 12.48 11.09   ~ 4243 3
3 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
4 QSO B0625-354 BLL 06 27 06.7286533392 -35 29 15.363665088   14.93       ~ 206 1
5 Z 184-50 BLL 11 04 27.3140835504 +38 12 31.798495872   13.50 12.90 8.31   ~ 2841 1
6 NGC 3862 Sy2 11 45 05.00904503 +19 36 22.7409909   14.98 13.97     ~ 646 1
7 M 87 AGN 12 30 49.42338414 +12 23 28.0436859 10.16 9.59 8.63   7.49 ~ 7815 3
8 NAME Centaurus A BLL 13 25 27.61521044 -43 01 08.8050291   8.18 6.84 6.66   ~ 4774 3

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