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2013 Sharon E. Meidt, Eva Schinnerer

ORCID

, Santiago García-Burillo, Annie Hughes, Dario Colombo, Jérôme Pety

ORCID

, Clare L. Dobbs, Karl F. Schuster, Carsten Kramer, Adam K. Leroy, Galle Dumas, Todd A. Thompson

Gas Kinematics on Giant Molecular Cloud Scales in M51 With Paws: Cloud Stabilization Through Dynamical Pressure

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Annie Hughes, Sharon E. Meidt, Dario Colombo, Eva Schinnerer

ORCID

ORCID

, Adam K. Leroy, Clare L. Dobbs, Santiago García-Burillo, Todd A. Thompson, Gaëlle Dumas, Karl F. Schuster, Carsten Kramer

A Comparative Study of Giant Molecular Clouds in M51, M33, and the Large Magellanic Cloud

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Annie Hughes, Sharon E. Meidt, Eva Schinnerer

ORCID

, Dario Colombo, Jerôme Pety, Adam K. Leroy, Clare L. Dobbs, Santiago García-Burillo, Todd A. Thompson, Gaëlle Dumas, Karl F. Schuster, Carsten Kramer

Probability Distribution Functions Of12co(j= 1 → 0) Brightness and Integrated Intensity in M51: The Paws View

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Eva Schinnerer

ORCID

, Sharon E. Meidt, Jérôme Pety

ORCID

, Annie Hughes, Dario Colombo, Santiago García-Burillo, Karl F. Schuster, Gaëlle Dumas, Clare L. Dobbs, Adam K. Leroy, Carsten Kramer, Todd A. Thompson, Michael W. Regan

The PdBI ARCSECOND WHIRLPOOL SURVEY (PAWS). I. A CLOUD-SCALE/MULTI-WAVELENGTH VIEW OF THE INTERSTELLAR MEDIUM IN a GRAND-DESIGN SPIRAL GALAXY

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Jérôme Pety

ORCID

, Eva Schinnerer

ORCID

, Adam K. Leroy, Annie Hughes, Sharon E. Meidt, Dario Colombo, Gaelle Dumas, Santiago García-Burillo, Karl F. Schuster, Carsten Kramer, Clare L. Dobbs, Todd A. Thompson

The PLATEAU DE BURE + 30 M ARCSECOND WHIRLPOOL SURVEY REVEALS a THICK DISK OF DIFFUSE MOLECULAR GAS IN THE M51 GALAXY

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Sandra P. Treviño-Morales

ORCID

, Asunción Fuente, Paolo Pilleri, Carsten Kramer, Manuel González-García, Evelyn Roueff, José Cernicharo, Jerome Pety

Study of deuterated molecules in the PDR around the UCHII region Mon R2

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Adam K. Leroy, Cheoljong Lee, Andreas Schruba, Alberto Bolatto, Annie Hughes, Jérôme Pety, Karin Sandstrom, Eva Schinnerer

ORCID

, Fabian Walter

ORCID

CLUMPING AND THE INTERPRETATION OF Kpc-Scale MAPS OF THE INTERSTELLAR MEDIUM: SMOOTH H I AND CLUMPY, VARIABLE H2SURFACE DENSITY

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