output
19922026
most citedSciPy 1.0--Fundamental Algorithms for Scientific Computing in Python

40.2k citations

Showing 2011 · astro-ph.GAShow all

14 papers · 2 filters

astro-ph.GA2011★ 35 cited

The APEX-CHAMP+ view of the Orion Molecular Cloud 1 core - Constraining the excitation with submillimeter CO multi-line observations

T. -C. Peng, F. Wyrowski, L. A. Zapata +2

A high density portion of the Orion Molecular Cloud 1 (OMC-1) contains the prominent, warm Kleinmann-Low (KL) nebula that is internally powered by an energetic event plus a farther…

astro-ph.GA2011★ 72 cited

Chemistry in Disks. V: CN and HCN in proto-planetary disks

E. Chapillon, S. Guilloteau, A. Dutrey +2

The chemistry of proto-planetary disks is thought to be dominated by two major processes: photodissociation near the disk surface, and depletion on dust grains in the disk mid-plan…

astro-ph.GA2011★ 14 cited

A Variable Star Census in a Perseus Field

T. Pasternacki, Sz. Csizmadia, J. Cabrera +13

The Berlin Exoplanet Search Telescope is a small-aperture, wide-field telescope dedicated to time-series photometric observations. During an initial commissioning phase at the Thue…

astro-ph.GA2011★ 240 cited

Filaments and ridges in Vela C revealed by Herschel: from low-mass to high-mass star-forming sites

Tracey Hill, Frederique Motte, Pierre Didelon +29

We present the first Herschel PACS and SPIRE results of the Vela C molecular complex in the far-infrared and submillimetre regimes at 70, 160, 250, 350, and 500 um, spanning the pe…

astro-ph.GA2011★ 20 cited

A deep search for H2D+ in protoplanetary disks

E. Chapillon, B. Parise, S. Guilloteau +1

The structure in density and temperature of protoplanetary disks surrounding low-mass stars is not yet well known. The protoplanetary disks mid-planes are expected to be very cold…

astro-ph.GA2011★ 49 cited

The Herschel M33 extended survey (HerM33es): PACS spectroscopy of the star forming region BCLMP 302

B. Mookerjea, C. Kramer, C. Buchbender +19

Context: The emission line of [CII] at 158 micron is one of the strongest cooling lines of the interstellar medium (ISM) in galaxies. Aims: Disentangling the relative contributions…