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Optical Dimming of RW Aur Associated with an Iron-rich Corona and Exceptionally High Absorbing Column Density

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Intensity-corrected Herschel Observations of Nearby Isolated Low-mass Clouds*

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The Power of SOFIA/FORCAST in Estimating Internal Luminosities of Low-mass Class 0/I Protostars

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Circumplanetary discs around young giant planets: a comparison between core-accretion and disc instability

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Characterizing the properties of cluster precursors in the MALT90 survey

Yanett Contreras, Jill M. Rathborne, Andres Guzman, et al.
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The turbulent life of dust grains in the supernova-driven, multiphase interstellar medium

Thomas Peters, Svitlana Zhukovska, Thorsten Naab, et al.
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Tracing the Magnetic Field of IRDC G028.23-00.19 Using NIR Polarimetry

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Constraining the Dust Opacity Law in Three Small and Isolated Molecular Clouds

K. A. Webb, J. Di Francesco, S. Sadavoy, K. Thanjavur, R. Launhardt, Y. Shirley, A. Stutz, J. Abreu Vicente and J. Kainulainen
The Astrophysical Journal 849 (1) 13 (2017)
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Properties of massive star-forming clumps with infall motions

Yu-Xin He, Jian-Jun Zhou, Jarken Esimbek, et al.
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High-resolution HI and CO observations of high-latitude intermediate-velocity clouds

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THE DISTRIBUTION OF MASS SURFACE DENSITIES IN A HIGH-MASS PROTOCLUSTER

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THE ORION H ii REGION AND THE ORION BAR IN THE MID-INFRARED

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THE HERSCHEL ORION PROTOSTAR SURVEY: SPECTRAL ENERGY DISTRIBUTIONS AND FITS USING A GRID OF PROTOSTELLAR MODELS

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X-RAY PROPERTIES OF LOW-MASS PRE-MAIN SEQUENCE STARS IN THE ORION TRAPEZIUM CLUSTER

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A SUB-ARCSECOND SURVEY TOWARD CLASS 0 PROTOSTARS IN PERSEUS: SEARCHING FOR SIGNATURES OF PROTOSTELLAR DISKS

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Smoke in the Pipe Nebula: dust emission and grain growth in the starless core FeSt 1-457

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CHARACTERIZING THE YOUNGESTHERSCHEL-DETECTED PROTOSTARS. I. ENVELOPE STRUCTURE REVEALED BY CARMA DUST CONTINUUM OBSERVATIONS

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Understanding the water emission in the mid- and far-IR from protoplanetary disks around T Tauri stars

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Dust evolution in the transition towards the denser ISM: impact on dust temperature, opacity, and spectral index

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