Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

ALMA Observations of DEM L241/LMC P3 in the Large Magellanic Cloud: Evidence for the Formation of Cool Molecular Jets Driven by a Microquasar

  • Authors: Yasuo Fukui, Bhuvana G. R., Hidetoshi Sano, Kisetsu Tsuge, Rami Z. E. Alsaberi, Rin Yamada, Yuya Asano, Aya Bamba, Miroslav Filipovic, Charles Law, Norikazu Mizuno, Toshikazu Onishi, Paul Plucinsky, Gavin Rowell, Manami Sasaki, Piyush Sharda, Hiromasa Suzuki, Kengo Tachihara, Kazuki Tokuda, Yumiko Yamane

Yasuo Fukui et al 2026 The Astrophysical Journal Letters 1011 .

  • Provider: AAS Journals

Caption: Figure 4.

Schematic side-view illustration of the large-scale geometry of the binary system and detected CO clouds within the SNR. The main molecular cloud is located in the foreground of the SNR and is surrounded by an envelope of H I gas. Interaction between the jet launched from the binary system and the ambient gas associated with this envelope is proposed to have produced the jet-like CO cloud located behind the main cloud.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse