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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 1.

(a) Multiwavelength overview of the SNR DEM L241 region. Red shows Chandra X-ray emission in 0.3−10 keV, green shows [S II] optical emission from DeMCELS, and blue shows Hα emission from DeMCELS. Overlaid contours represent ASTE 12CO(J=3–2) emission. The yellow box indicates the ALMA ACA observation mosaic region. (b) ALMA 12CO(J=3–2) emission integrated over the velocity range 285.6−288.0 km s−1 that shows jet clouds. The contour shows the ALMA 12CO(J=3–2) emission integrated over the velocity range 279.6–283.6 km s−1, representing the ambient molecular cloud, at a significance level of 3σ. The position of the point source is marked with a star symbol.

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