The jet collimation profile at high resolution in BL Lacertae
Artikel i vetenskaplig tidskrift, 2021
Context. Controversial studies on the jet collimation profile of BL Lacertae (BL Lac), the eponymous blazar of the BL Lac objects class, complicate the scenario in this already puzzling class of objects. Understanding the jet geometry in connection with the jet kinematics and the physical conditions in the surrounding medium is fundamental for better constraining the formation, acceleration, and collimation mechanisms in extragalactic jets. Aims. With the aim of investigating the jet geometry in the innermost regions of the BL Lac jet, and resolving the controversy, we explore the radio jet in this source using high-resolution millimeter-wave VLBI data. Methods. We collect 86 GHz GMVA and 43 GHz VLBA data to obtain stacked images that we use to infer the jet collimation profile by means of two comparable methods. We analyze the kinematics at 86 GHz, and we discuss it in the context of the jet expansion. Finally, we consider a possible implication of the Bondi sphere in shaping the jet of BL Lac. Results. The jet in BL Lac expands with an overall conical geometry. A higher expanding rate region is observed between ∼5 and 10 pc (de-projected) from the black hole. Such a region is associated with the decrease in brightness usually observed in high-frequency VLBI images of BL Lac. The jet retrieves the original jet expansion around 17 pc, where the presence of a recollimation shock is supported by both the jet profile and the 15 GHz kinematics (MOJAVE survey). The change in the jet expansion profile occurring at ∼5 pc could be associated with a change in the external pressure at the location of the Bondi radius (∼3.3 × 105RS).
Instrumentation: high angular resolution
Instrumentation: interferometers
Galaxies: jets
BL Lacertae objects: individual: BL Lacertae
Galaxies: active
Författare
C. Casadio
Idryma Technologias kai Erevnas (FORTH)
Max-Planck-Gesellschaft
N. R. Macdonald
Max-Planck-Gesellschaft
B. Boccardi
Max-Planck-Gesellschaft
S.G. Jorstad
Saint Petersburg State University - Spsu
Boston University
A. Marscher
Boston University
T.P. Krichbaum
Max-Planck-Gesellschaft
J. Hodgson
Sejong University
Jae-Young Kim
Korea Astronomy and Space Science Institute
Max-Planck-Gesellschaft
E. Traianou
Max-Planck-Gesellschaft
Z. R. Weaver
Boston University
M. Gómez Garrido
Centro de Desarrollos Tecnológicos
J. González García
Centro de Desarrollos Tecnológicos
J. Kallunki
Aalto-Yliopisto
Michael Lindqvist
Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium
S. Sánchez
Instituto de Radio Astronomía Millimétrica
Jun Yang
Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium
A.J. Zensus
Max-Planck-Gesellschaft
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 649 A153Ämneskategorier
Astronomi, astrofysik och kosmologi
Geofysik
Fusion, plasma och rymdfysik
DOI
10.1051/0004-6361/202039616