Optical IFU spectroscopy of a bipolar microquasar jet in NGC 300. Issue 3 (2nd March 2019)

• Record Type: Journal Article
• Authors: McLeod, A F; Scaringi, S; Soria, R; Pakull, M W; Urquhart, R; Maccarone, T J; Knigge, C; Miller-Jones, J C A; Plotkin, R M; Motch, C; Kruijssen, J M D; Schruba, A
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 485:Issue 3(2019)
• Page Start: 3476
• Page End: 3485
• Publication Date: 2019-03-02
• Subjects: accretion, accretion discs -- black hole physics -- X-rays: binaries; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stz614
• Languages: English
• ISSNs: 0035-8711

Abstract

Abstract: We recently reported the discovery of a candidate jet-driving microquasar (S10) in the nearby spiral galaxy NGC 300. However, in the absence of kinematic information, we could not reliably determine the jet power or the dynamical age of the jet cavity. Here, we present optical Multi Unit Spectroscopic Explorer (MUSE) integral field unit (IFU) observations of S10, which reveal a bipolar line-emitting jet structure surrounding a continuum-emitting central source. The optical jet lobes of S10 have a total extent of ∼40 pc and a shock velocity of ∼150 km s −1 . Together with the jet kinematics, we exploit the MUSE coverage of the Balmer Hβ line to estimate the density of the surrounding matter and therefore compute the jet power to be P jet ≈ 6.3 × 10 38 erg s −1 . An optical analysis of a microquasar jet bubble and a consequent robust derivation of the jet power have been possible only in a handful of similar sources. This study therefore adds valuable insight into microquasar jets, and demonstrates the power of optical integral field spectroscopy in identifying and analysing these objects.