IPA. Accretion rate of a low-mass Class 0 protostar, measured via mid-infrared fluorescent OH emission

D. M. Watson(University of Rochester), William J. Fischer(Space Telescope Science Institute), John Tobin(Leiden University), Joel D. Green(Space Telescope Science Institute), Robert Gutermuth(University of Massachusetts Amherst), Samuel Federman(Astronomical Observatory of Capodimonte), A. Caratti o Garatti(Dublin Institute For Advanced Studies), Nolan Habel(University of Toledo), H. Linz(Max Planck Institute for Astronomy), Łukasz Tychoniec(European Southern Observatory), Nashanty G. C. Brunken(Leiden University), Tyler L. Bourke(University of Manchester), Prabhani Atnagulov, Thomas Stanke, S. T. Megeath(University of Toledo), Caeley V. Pittman(Boston University), Pamela Klaassen, Yao-Lun Yang(Korea Astronomy and Space Science Institute), James Muzerolle Page, Mayank Narang, Adam E. Rubinstein, E. F. van Dishoeck(Leiden University), Leslie W. Looney(University of Illinois Urbana-Champaign), David A. Neufeld(Johns Hopkins University), H. Beuther(Max Planck Institute for Astronomy), Elise Furlan(Jet Propulsion Laboratory), Rohan Rahatgaonkar, W. R. M. Rocha(Leiden University), Guillem Anglada(Instituto de Astrofísica de Andalucía), C. M. Lisse(Johns Hopkins University Applied Physics Laboratory), Amelia M. Stutz(University of Concepción), Nicole Karnath(University of Toledo), Catherine Espaillat, K. Slavicinska(Leiden University), Neal J. Evans(The University of Texas at Austin), Nuria Calvet(Center for Astrophysics Harvard & Smithsonian), Patrick Sheehan, Mayra Osorio(Instituto de Astrofísica de Andalucía), Himanshu Tyagi(Tata Institute of Fundamental Research), Pooneh Nazari(Leiden University), Lee W. Hartmann, Riwaj Pokhrel(University of Massachusetts Amherst)
arXiv (Cornell University)
December 17, 2025
Cited by 1


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