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Moscadelli, L · 2011

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astro-ph.SR 1

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2026 1

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CONDITIONAL 1

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Evidence for a bloated massive protostar in IRAS20126+4104

astro-ph.SR · 2026-04-14 · conditional · novelty 4.0

Mid-IR light curves of IRAS20126+4104 confirm a 6.8 yr periodic variation interpreted as evidence that the 12 solar-mass protostar is bloated to a radius of roughly 200 solar radii due to rotation with an obscuring spot.

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  • Evidence for a bloated massive protostar in IRAS20126+4104 astro-ph.SR · 2026-04-14 · conditional · none · ref 25

    Mid-IR light curves of IRAS20126+4104 confirm a 6.8 yr periodic variation interpreted as evidence that the 12 solar-mass protostar is bloated to a radius of roughly 200 solar radii due to rotation with an obscuring spot.