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Cited article:

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AN IMPRINT OF MOLECULAR CLOUD MAGNETIZATION IN THE MORPHOLOGY OF THE DUST POLARIZED EMISSION

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The mid-infrared extinction law in the darkest cores of the Pipe Nebula

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LINE PROFILES OF CORES WITHIN CLUSTERS. II. SIGNATURES OF DYNAMICAL COLLAPSE DURING HIGH-MASS STAR FORMATION

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Herschelview of the Taurus B211/3 filament and striations: evidence of filamentary growth?

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YOUNG STARLESS CORES EMBEDDED IN THE MAGNETICALLY DOMINATED PIPE NEBULA. II. EXTENDED DATA SET

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THE ROLE OF θ OPH IN THE FORMATION AND EVOLUTION OF THE PIPE NEBULA—IS STAR FORMATION EVER ISOLATED?

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THE STAR FORMATION RATE OF TURBULENT MAGNETIZED CLOUDS: COMPARING THEORY, SIMULATIONS, AND OBSERVATIONS

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STABLE AND UNSTABLE EQUILIBRIA OF UNIFORMLY ROTATING SELF-GRAVITATING CYLINDERS

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