An ALMA view of the Jet-Arc CO clouds toward the TeV γ-ray source HESS J1023-575 and Westerlund 2; Evidence for the footprints of microquasar jets, the very powerful cosmic-ray accelerator in the Galactic disk

@misc{fukui2026alma,
  title = {{An ALMA view of the Jet-Arc CO clouds toward the TeV $γ$-ray source HESS J1023-575 and Westerlund 2; Evidence for the footprints of microquasar jets, the very powerful cosmic-ray accelerator in the Galactic disk}},
  author = {Yasuo Fukui and Kisetsu Tsuge and Hidetoshi Sano and G. R. Bhuvana and Rin I. Yamada and Ryoji Matsumoto and Yuta Asahina and Tsuyoshi Inoue and Tim Lukas Holch and Emma de Oña Wilhelmi},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2608.14988},
  eprint = {2608.14988},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2608.14988},
}

TY  - UNPB
TI  - An ALMA view of the Jet-Arc CO clouds toward the TeV γ-ray source HESS J1023-575 and Westerlund 2; Evidence for the footprints of microquasar jets, the very powerful cosmic-ray accelerator in the Galactic disk
AU  - Yasuo Fukui
AU  - Kisetsu Tsuge
AU  - Hidetoshi Sano
AU  - G. R. Bhuvana
AU  - Rin I. Yamada
AU  - Ryoji Matsumoto
AU  - Yuta Asahina
AU  - Tsuyoshi Inoue
AU  - Tim Lukas Holch
AU  - Emma de Oña Wilhelmi
PY  - 2026
DA  - 2026/09/14
PB  - arXiv
DO  - 10.48550/arxiv.2608.14988
UR  - https://arxiv.org/abs/2608.14988
AB  - The TeV γ-ray source HESS J1023-575 (HESSJ 1023 hereafter) is one of the brightest H.E.S.S. sources near the young massive cluster Westerlund 2. HESS J1023 shows a remarkable positional alignment with the Jet and Arc CO clouds on its eastern and western sides over 170 pc length. We have carried out sub-pc scale observations of the CO clouds with ALMA and have discovered that the clouds consist of numerous thin filamentary features of ∼0.5 pc width and 10--20 pc length at distance of 7.5 kpc, which are well aligned with the Jet-Arc axis. Based on the magneto-hydrodynamical model of microquasar jets launched from {the center of the γ-ray source} HESS J1023-575, we present an interpretation that the thin filamentary clouds are the footprints of the microquasar jets on the HI gas. The model also explains the dissimilar Jet vs. Arc clouds in terms of HI density difference on each side. By using the density of the CO and HI gas and the γ-ray luminosity, we have calculated the cosmic ray proton energy W_p to be 7×10^48 erg under the hadronic scheme, which is ten times larger than those derived in the TeV γ-ray SNRs RX J1713.7-3946 and RX J0852.0-4622. It is likely that HESS~J1023 has been active over 1-10 Myr, which is significantly longer than the duration of cosmic ray acceleration of the SNRs. HESS~J1023 is therefore an outstanding source of cosmic rays equivalent to at least 1000 SNRs, and is possibly the most powerful CR accelerator in the Galactic disk. A high energy compact source in HESS~J1023, which is likely a Myr-old black hole or neutron star, remains veiled due to heavy extinction.
ER  -