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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 3.

(a) Intensity map of jet clouds in velocity range 285−289 km s⁻¹. The boxes indicate the pixel regions selected for estimating physical properties. (b) Kinetic temperature of jet clouds BC and D along with the ambient cloud estimated in this study are plotted against their density. The horizontal dotted lines indicate the typical temperature range of unshocked cloud in LMC including the uncertainties.

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