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Infrared radiation feedback does not regulate star cluster formation
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Philip F Hopkins, Anna L Rosen, Jonathan Squire, Georgia V Panopoulou, Nadine H Soliman, Darryl Seligman and Ulrich P Steinwandel Monthly Notices of the Royal Astronomical Society 517(1) 1491 (2022) https://doi.org/10.1093/mnras/stac1784
VETTAM: a scheme for radiation hydrodynamics with adaptive mesh refinement using the variable Eddington tensor method
Shyam H Menon, Christoph Federrath, Mark R Krumholz, et al. Monthly Notices of the Royal Astronomical Society 512(1) 401 (2022) https://doi.org/10.1093/mnras/stac485
Super-Eddington Mass Growth of Intermediate-mass Black Holes Embedded in Dusty Circumnuclear Disks
Formation of massive stars under protostellar radiation feedback: very metal-poor stars
Hajime Fukushima, Takashi Hosokawa, Gen Chiaki, et al. Monthly Notices of the Royal Astronomical Society 497(1) 829 (2020) https://doi.org/10.1093/mnras/staa1994
A new hybrid radiative transfer method for massive star formation
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Philip F Hopkins, Michael Y Grudić, Andrew Wetzel, et al. Monthly Notices of the Royal Astronomical Society 491(3) 3702 (2020) https://doi.org/10.1093/mnras/stz3129
Gaseous dynamical friction under radiative feedback: do intermediate-mass black holes speed up or down?
Rolf Kuiper, Kazuyuki Sugimura, Takashi Hosokawa and Daisuke Toyouchi Monthly Notices of the Royal Astronomical Society 496(2) 1909 (2020) https://doi.org/10.1093/mnras/staa1338
Zooming in on Individual Star Formation: Low- and High-Mass Stars
arepo-rt: radiation hydrodynamics on a moving mesh
Rahul Kannan, Mark Vogelsberger, Federico Marinacci, et al. Monthly Notices of the Royal Astronomical Society 485(1) 117 (2019) https://doi.org/10.1093/mnras/stz287
Forming spectroscopic massive protobinaries by disc fragmentation
D. M.-A. Meyer, R. Kuiper, W. Kley, K. G. Johnston and E. Vorobyov Monthly Notices of the Royal Astronomical Society 473(3) 3615 (2018) https://doi.org/10.1093/mnras/stx2551
The resonant drag instability (RDI): acoustic modes
Upper stellar mass limit by radiative feedback at low-metallicities: metallicity and accretion rate dependence
Hajime Fukushima, Kazuyuki Omukai and Takashi Hosokawa Monthly Notices of the Royal Astronomical Society 473(4) 4754 (2018) https://doi.org/10.1093/mnras/stx2620
A Review of the Theory of Galactic Winds Driven by Stellar Feedback
Radiation Hydrodynamics Simulations of Photoevaporation of Protoplanetary Disks by Ultraviolet Radiation: Metallicity Dependence
Riouhei Nakatani, Takashi Hosokawa, Naoki Yoshida, Hideko Nomura and Rolf Kuiper The Astrophysical Journal 857(1) 57 (2018) https://doi.org/10.3847/1538-4357/aab70b
Radiation-hydrodynamical simulations of massive star formation using Monte Carlo radiative transfer – II. The formation of a 25 solar-mass star
Tim J. Harries, Tom A. Douglas and Ahmad Ali Monthly Notices of the Royal Astronomical Society 471(4) 4111 (2017) https://doi.org/10.1093/mnras/stx1490
Radiation feedback in dusty clouds
Shohei Ishiki and Takashi Okamoto Monthly Notices of the Royal Astronomical Society: Letters 466(1) L123 (2017) https://doi.org/10.1093/mnrasl/slw253
Fragmentation and disk formation in high-mass star formation: The ALMA view of G351.77-0.54 at 0.06′′ resolution
On the observability of bow shocks of Galactic runaway OB stars
D. M.-A. Meyer, A.-J. van Marle, R. Kuiper and W. Kley Monthly Notices of the Royal Astronomical Society 459(2) 1146 (2016) https://doi.org/10.1093/mnras/stw651
PROTOSTELLAR OUTFLOWS AND RADIATIVE FEEDBACK FROM MASSIVE STARS. II. FEEDBACK, STAR-FORMATION EFFICIENCY, AND OUTFLOW BROADENING
An unstable truth: how massive stars get their mass
Anna L. Rosen, Mark R. Krumholz, Christopher F. McKee and Richard I. Klein Monthly Notices of the Royal Astronomical Society 463(3) 2553 (2016) https://doi.org/10.1093/mnras/stw2153
SIMULATING THE FORMATION OF MASSIVE PROTOSTARS. I. RADIATIVE FEEDBACK AND ACCRETION DISKS
T. G. Bisbas, T. J. Haworth, R. J. R. Williams, et al. Monthly Notices of the Royal Astronomical Society 453(2) 1324 (2015) https://doi.org/10.1093/mnras/stv1659
Fervent: chemistry-coupled, ionizing and non-ionizing radiative feedback in hydrodynamical simulations
C. Baczynski, S. C. O. Glover and R. S. Klessen Monthly Notices of the Royal Astronomical Society 454(1) 380 (2015) https://doi.org/10.1093/mnras/stv1906
Radiation-hydrodynamical simulations of massive star formation using Monte Carlo radiative transfer – I. Algorithms and numerical methods
Rolf Kuiper, Hubert Klahr, Henrik Beuther and Thomas Henning Astrophysics and Space Science Proceedings, The Labyrinth of Star Formation 36 379 (2014) https://doi.org/10.1007/978-3-319-03041-8_74
Morphologies of protostellar outflows: an ALMA view
Thomas Peters, Pamela D. Klaassen, Daniel Seifried, Robi Banerjee and Ralf S. Klessen Monthly Notices of the Royal Astronomical Society 437(3) 2901 (2014) https://doi.org/10.1093/mnras/stt2104
The Labyrinth of Star Formation
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A GENERAL HYBRID RADIATION TRANSPORT SCHEME FOR STAR FORMATION SIMULATIONS ON AN ADAPTIVE GRID
Radiation pressure confinement – III. The origin of the broad ionization distribution in AGN outflows
Jonathan Stern, Ehud Behar, Ari Laor, Alexei Baskin and Tomer Holczer Monthly Notices of the Royal Astronomical Society 445(3) 3011 (2014) https://doi.org/10.1093/mnras/stu1960
Galaxies on FIRE (Feedback In Realistic Environments): stellar feedback explains cosmologically inefficient star formation
Philip F. Hopkins, Dušan Kereš, José Oñorbe, et al. Monthly Notices of the Royal Astronomical Society 445(1) 581 (2014) https://doi.org/10.1093/mnras/stu1738
Rayleigh–Taylor instability of ionization front around black holes
KwangHo Park, Massimo Ricotti, Tiziana Di Matteo and Christopher S. Reynolds Monthly Notices of the Royal Astronomical Society 437(3) 2856 (2014) https://doi.org/10.1093/mnras/stt2096
Numerical simulations of radiatively driven dusty winds
Dense molecular gas: a sensitive probe of stellar feedback models
Philip F. Hopkins, Desika Narayanan, Norman Murray and Eliot Quataert Monthly Notices of the Royal Astronomical Society 433(1) 69 (2013) https://doi.org/10.1093/mnras/stt688
Radiation hydrodynamics integrated in the PLUTO code
ARE MOLECULAR OUTFLOWS AROUND HIGH-MASS STARS DRIVEN BY IONIZATION FEEDBACK?
Thomas Peters, Pamela D. Klaassen, Mordecai-Mark Mac Low, Ralf S. Klessen and Robi Banerjee The Astrophysical Journal 760(1) 91 (2012) https://doi.org/10.1088/0004-637X/760/1/91
WEAKLY INTERACTING MASSIVE PARTICLE DARK MATTER AND FIRST STARS: SUPPRESSION OF FRAGMENTATION IN PRIMORDIAL STAR FORMATION
Stellar feedback and bulge formation in clumpy discs
Philip F. Hopkins, Dusan Kereš, Norman Murray, Eliot Quataert and Lars Hernquist Monthly Notices of the Royal Astronomical Society 427(2) 968 (2012) https://doi.org/10.1111/j.1365-2966.2012.21981.x
THE GROWTH OF THE STELLAR SEEDS OF SUPERMASSIVE BLACK HOLES