First results from the Herschel Gould Belt Survey in Taurus

@article{Kirk2013FirstRF,
  title={First results from the Herschel Gould Belt Survey in Taurus},
  author={Jason M. Kirk and Derek Ward-Thompson and Pedro Palmeirim and Ph. Andre' and Matthew Joseph Griffin and P. Hargrave and Vera Konyves and J-Ph. Bernard and David John Nutter and Bruce Sibthorpe and James Di Francesco and Alain Abergel and Doris Arzoumanian and Milena Benedettini and Sylvain Bontemps and Davide Elia and Martin Hennemann and T. Hill and A.Men'shchikov and F.Motte and Quang Nguyen-Luong and Nicolas Peretto and Stefano Pezzuto and Kazi L. J. Rygl and Sarah I. Sadavoy and Eugenio Schisano and Nicola Schneider and Leonardo Testi and GA 30332-0430 School of Physics and Astronomy and Cardiff University and UK. and Jeremiah Horrocks Institute and Preston and UK Laboratoire Aim and Sea Saclay and France. and Cnrs and Toulouse and Universit'e de Toulouse and UK Atc and Royal Observatory of Edinburgh and NRCC-HIA and Victoria and Canada. and Dep. of Physics and University of Victoria and Institut d'Astrophysique Spatiale and Orsay and Istituto di Astrofisica e Planetologia Spaziali and Roma and Italy. and Universit'e de Bordeaux and Bordeaux and Canadian Institute for Theoretical Astrophysics and University of Toronto and Eső and Garching and H Germany and Rutherford Appleton Laboratory and The Open University},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2013},
  volume={432},
  pages={1424-1433}
}
The whole of the Taurus region (a total area of 52 deg2) has been observed by the Herschel Spectral and Photometric Imaging Receiver (SPIRE) and Photodetector Array Camera and Spectrometer (PACS) instruments at wavelengths of 70, 160, 250, 350 and 500 μm as part of the Herschel Gould Belt Survey. In this paper we present the first results from the part of the Taurus region that includes the Barnard 18 and L1536 clouds. A new source-finding routine, the Cardiff Source-finding AlgoRithm (csar… 

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References

SHOWING 1-10 OF 65 REFERENCES
Initial highlights from the Herschel Gould Belt survey
We summarize the first results from the Gould Belt survey, obtained toward the Aquila Rift and Polaris Flare regions during the 'science demonstration phase' of Herschel. Our 70-500 micron images
Large-Scale Structure of the Molecular Gas in Taurus Revealed by High Linear Dynamic Range Spectral Line Mapping
We report the results of a 100 deg2 survey of the Taurus molecular cloud region in 12CO and 13CO J = 1→ 0. The image of the cloud in each velocity channel includes ≃3 × 106 Nyquist-sampled pixels on
The Herschel view of the on-going star formation in the Vela-C molecular cloud
Aims. As part of the Herschel guaranteed time key programme “HOBYS”, we present the PACS and SPIRE photometric survey of the star-forming region Vela-C, one of the nearest sites of low-to-high-mass
Herschel view of the Taurus B211/3 filament and striations: evidence of filamentary growth?
We present first results from the Herschel Gould Belt survey for the B211/L1495 region in the Taurus molecular cloud. Thanks to their high sensitivity and dynamic range, the Herschel images reveal
A Herschel study of the properties of starless cores in the Polaris Flare dark cloud region using PACS and SPIRE
The Polaris Flare cloud region contains a great deal of extended emission. It is at high declination and high Galactic latitude. It was previously seen strongly in IRAS Cirrus emission at 100
CO Isotopologues in the Perseus Molecular Cloud Complex: the X-factor and Regional Variations
We use data gathered by the COMPLETE survey of star-forming regions to find new calibrations of the “X-factor” and 13CO abundance within the Perseus molecular cloud. We divide Perseus into six
Mapping the column density and dust temperature structure of IRDCs with Herschel
Infrared dark clouds (IRDCs) are cold and dense reservoirs of gas potentially available to form stars. Many of these clouds are likely to be pristine structures representing the initial conditions
A Complete Search for Dense Cloud Cores in Taurus
We present the results of an H13CO+ J = 1-0 survey for dense molecular condensations in Taurus. The observations were carried out with the 45 m telescope at Nobeyama on the basis of an extensive C18O
A SCUBA survey of the NGC 2068/2071 protoclusters
We report the results of a submillimeter dust continuum survey of the protoclusters NGC 2068 and NGC 2071 in Orion B carried out at 850 m and 450 m with SCUBA on JCMT. The mapped region is32 0 18 0
MEASURING THE CLUMP MASS FUNCTION IN THE AGE OF SCUBA2, HERSCHEL, AND ALMA
We use simulated images of star-forming regions to explore the effects of various image acquisition techniques on the derived clump mass function. In particular, we focus on the effects of finite
...
...