Turn up the light: Radiative efficiency of protostars at birth
Abstract
The early stages of stellar birth comprise a two-step process involving the formation of two hydrostatic cores. The second step of gravitational collapse sets the radiative efficiency and accretion rate of the young protostar. These two parameters, which are of prime importance for protostellar evolution, dictate the luminosities and thus play a key role in deciphering the current discrepancy between observational surveys and theoretical models. In this Letter, we provide quantitative estimates on the evolution of the radiative efficiency and accretion rate obtained from self-consistent, high-resolution, radiative hydrodynamic simulations performed using the codes PLUTO and RAMSES . The main highlight of our result is that the radiative efficiency reaches unity, that is, supercriticality, relatively quickly after protostellar birth. Supercriticality at the accretion shock is a necessary condition for cold accretion. Our results thus support a rapid transition to the cold accretion scenario, which is one of the assumptions used in pre-main sequence (PMS) models when working towards solutions to explain observational data. We briefly discuss the implications of the time evolution of the radiative efficiency factor in the context of the luminosity problem, the protostellar luminosity function, PMS evolution, accurate sink properties, and the stellar initial mass function.
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BibTeX
@article{bhandare2026turn,
title = {{Turn up the light: Radiative efficiency of protostars at birth}},
author = {Asmita Bhandare and Adnan Ali Ahmad and Benoît Commerçon},
journal = {Astronomy \& Astrophysics - A\&A},
year = {2026},
month = sep,
doi = {10.1051/0004-6361/202556128},
url = {https://hal.science/hal-05737395v1},
note = {CC BY-NC-ND 4.0},
}
RIS
TY - JOUR
TI - Turn up the light: Radiative efficiency of protostars at birth
AU - Asmita Bhandare
AU - Adnan Ali Ahmad
AU - Benoît Commerçon
PY - 2026
DA - 2026/09/03
JO - Astronomy & Astrophysics - A&A
DO - 10.1051/0004-6361/202556128
UR - https://hal.science/hal-05737395v1
AB - The early stages of stellar birth comprise a two-step process involving the formation of two hydrostatic cores. The second step of gravitational collapse sets the radiative efficiency and accretion rate of the young protostar. These two parameters, which are of prime importance for protostellar evolution, dictate the luminosities and thus play a key role in deciphering the current discrepancy between observational surveys and theoretical models. In this Letter, we provide quantitative estimates on the evolution of the radiative efficiency and accretion rate obtained from self-consistent, high-resolution, radiative hydrodynamic simulations performed using the codes PLUTO and RAMSES . The main highlight of our result is that the radiative efficiency reaches unity, that is, supercriticality, relatively quickly after protostellar birth. Supercriticality at the accretion shock is a necessary condition for cold accretion. Our results thus support a rapid transition to the cold accretion scenario, which is one of the assumptions used in pre-main sequence (PMS) models when working towards solutions to explain observational data. We briefly discuss the implications of the time evolution of the radiative efficiency factor in the context of the luminosity problem, the protostellar luminosity function, PMS evolution, accurate sink properties, and the stellar initial mass function.
SN - 0004-6361
SN - 1432-0746
ER -