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The Fraction of Dust Mass in the Form of Polycyclic Aromatic Hydrocarbons on 10–50 pc Scales in Nearby Galaxies
Jessica Sutter, Karin Sandstrom, Jérémy Chastenet, Adam K. Leroy, Eric W. Koch, Thomas G. Williams, Ryan Chown, Francesco Belfiore, Frank Bigiel, Médéric Boquien, Yixian Cao, Mélanie Chevance, Daniel A. Dale, Oleg V. Egorov, Simon C. O. Glover, Brent Groves, Ralf S. Klessen, Kathryn Kreckel, Kirsten L. Larson, Elias K. Oakes, Debosmita Pathak, Lise Ramambason, Erik Rosolowsky and Elizabeth J. Watkins The Astrophysical Journal 971(2) 178 (2024) https://doi.org/10.3847/1538-4357/ad54bd
Constraining the H2 column densities in the diffuse interstellar medium using dust extinction and H I data
Dust in the wind with resonant drag instabilities – I. The dynamics of dust-driven outflows in GMCs and H ii regions
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
HI-H2 transition: Exploring the role of the magnetic field
The dynamics of charged dust in magnetized molecular clouds
Hyunseok Lee, Philip F. Hopkins and Jonathan Squire Monthly Notices of the Royal Astronomical Society 469(3) 3532 (2017) https://doi.org/10.1093/mnras/stx1097
Are the Formation and Abundances of Metal-poor Stars the Result of Dust Dynamics?
Formation history of polycyclic aromatic hydrocarbons in galaxies
Ji Yeon Seok, Hiroyuki Hirashita and Ryosuke S. Asano Monthly Notices of the Royal Astronomical Society 439(2) 2186 (2014) https://doi.org/10.1093/mnras/stu120
SOME STARS ARE TOTALLY METAL: A NEW MECHANISM DRIVING DUST ACROSS STAR-FORMING CLOUDS, AND CONSEQUENCES FOR PLANETS, STARS, AND GALAXIES
THESPITZERSURVEY OF THE SMALL MAGELLANIC CLOUD (S3MC): INSIGHTS INTO THE LIFE CYCLE OF POLYCYCLIC AROMATIC HYDROCARBONS
Karin M. Sandstrom, Alberto D. Bolatto, B. T. Draine, Caroline Bot and Snežana Stanimirović The Astrophysical Journal 715(2) 701 (2010) https://doi.org/10.1088/0004-637X/715/2/701
DUST IN THE DIFFUSE EMISSION OF THE GALACTIC PLANE: THE
HERSCHEL
/
SPITZER
SPECTRAL ENERGY DISTRIBUTION FITTING
Soft X-Ray Emission from Clusters of Galaxies and Related Phenomena
Felix J. Lockman Astrophysics and Space Science Library, Soft X-Ray Emission from Clusters of Galaxies and Related Phenomena 309 111 (2004) https://doi.org/10.1007/978-1-4020-2564-8_13
On the Use of Fractional Brownian Motion Simulations to Determine the Three‐dimensional Statistical Properties of Interstellar Gas
M.‐A. Miville‐Deschenes, F. Levrier and E. Falgarone The Astrophysical Journal 593(2) 831 (2003) https://doi.org/10.1086/376603
Dust emission from inhomogeneous interstellar clouds:
Radiative transfer in 3D with transiently heated particles