A dataset provided by the European Space Agency

Name OT1_pharve01_3
Title The Auriga-California Molecular Cloud: A Massive Nearby Cloud With Powerful Diagnostics For Early Stages of Star Formation
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342239276&instrument_name=SPIRE\/PACS parallel&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342239276&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342239277&instrument_name=SPIRE\/PACS parallel&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342239277&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342239278&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342239278&instrument_name=SPIRE\/PACS parallel&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342239279&instrument_name=SPIRE\/PACS parallel&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342239279&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342239441&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342239441&instrument_name=SPIRE\/PACS parallel&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342239442&instrument_name=SPIRE\/PACS parallel&product_level=LEVEL0&compress=true
...
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342239442&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342240279&instrument_name=SPIRE\/PACS parallel&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342240279&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342240314&instrument_name=SPIRE\/PACS parallel&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342240314&instrument_name=PACS&product_level=LEVEL0&compress=true

DOI 10.5270/esa-2o2mdbq
Author harvey, p.
Description We propose to map the Auriga-California Molecular Cloud (AMC) with the same observing parameters as being used for the rest of the clouds in the Gould Belt by the Herschel GT team conducting that program. The AMC was not included in that program BUT is extremely important as a counterpoint to the Orion Molecular Cloud (OMC) because it is as large and massive as the OMC but has a factor of 10 lower level of star formation, most of which is concentrated at the southeast end near the LkHalpha 101 cluster. We already have complete Spitzer survey data on this cloud and are in the process of obtaining JCMT line and continuum survey observations. The OMC has informed our understanding of star clusters and massive star formation. It is essential, however, to test that understanding by observing other massive clouds with differing levels of star formation. The combination of Herschel data with our existing Spitzer and molecular line data is vital to understand the physical reasons underlying the large differences in star formation between these two regions. Herschel.s combination of angular resolution and 5-band imaging for dust temperature and emissivity measurements permit a uniquely high level of analysis of the far-IR emission from the AMC and comparison with the OMC.
Publication Physical properties and chemical composition of the cores in the California molecular cloud . Zhang Guo-Yin et al. . Astronomy & Astrophysics, Volume 620, id.A163, 22 pp. . 620 . 10.1051\/0004-6361\/201833622 . 2018A&A...620A.163Z ,
Filament identification through mathematical morphology . Koch Eric W. et al. . Monthly Notices of the Royal Astronomical Society, Volume 452, Issue 4, p.3435-3450 . 452 . 10.1093\/mnras\/stv1521 . 2015MNRAS.452.3435K ,
The JCMT Gould Belt Survey: A First Look at the Auriga–California Molecular Cloud with SCUBA-2 . Broekhoven-Fiene H. et al. . The Astrophysical Journal, Volume 852, Issue 2, article id. 73, 20 pp. (2018). . 852 . 10.3847\/1538-4357\/aa911f . 2018ApJ...852...73B ,
Understanding star formation in molecular clouds. I. Effects of line-of-sight contamination on the column density structure . Schneider N. et al. . Astronomy & Astrophysics, Volume 575, id.A79, 17 pp. . 575 . 10.1051\/0004-6361\/201423569 . 2015A&A...575A..79S ,
Herschel and SCUBA-2 observations of dust emission in a sample of Planck cold clumps . Juvela Mika et al. . Astronomy & Astrophysics, Volume 612, id.A71, 38 pp. . 612 . 10.1051\/0004-6361\/201731921 . 2018A&A...612A..71J ,
Relationship between turbulence energy and density variance in the solar neighbourhood molecular clouds . Kainulainen J. et al. . Astronomy & Astrophysics, Volume 608, id.L3, 6 pp. . 608 . 10.1051\/0004-6361\/201731028 . 2017A&A...608L...3K ,
HP2 survey. III. The California Molecula...
Instrument PACS_PacsPhoto_largeScan, SPIRE\/PACS parallel_SpirePacsParallel_
Temporal Coverage 2012-02-13T19:23:01Z/2012-03-05T18:48:48Z
Version SPG v14.2.0
Mission Description Herschel was launched on 14 May 2009! It is the fourth 'cornerstone' mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 µm range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/herschel/
Date Published 2012-09-05T16:31:27Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-09-05T16:31:27Z, OT1_pharve01_3, SPG v14.2.0. https://doi.org/10.5270/esa-2o2mdbq