A dataset provided by the European Space Agency

Name OT1_rgutermu_1
Title A Herschel SPIRE/PACS Imaging Survey of the MonR2 and CepOB3 Molecular Clouds

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342263817&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=1342263818&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=1342263852&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=1342263853&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=1342267715&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=1342267746&instrument_name=SPIRE\/PACS parallel&product_level=LEVEL0&compress=true

DOI https://doi.org/10.5270/esa-nbrzx4r
Author gutermuth, r.
Description We propose complete surveys of the MonR2 (830 pc) and CepOB3 (700 pc) molecular
clouds with SPIRE and PACS on Herschel to complement extant surveys with
NEWFIRM and Spitzer at near-IR and mid-IR wavelengths, respectively. These two
clouds complement cloud surveys of Orion and the Gould Belt clouds, as they are
actively forming both low and high mass stars, and they are found at different
evolutionary states relative to Orion. They are also closer to the galactic
plane than Orion, implying a higher density of background stars and more
reliable extinction maps. This study will impact our knowledge of two
essential problems in star formation: the physical factors which determine the
star formation rate and the initial mass function. We will produce high
resolution maps of the large-scale dust column density and temperature from the
SPIRE data maps and compare these to the density of protostars to determine the
rate of star formation per area relative to the gas column density. We will
use this data to reconcile inconsistent star formation rate vs gas column
density correlations recently reported in the literature by measuring this
relationship by independent means in a single cloud. To study the IMF, and its
possible dependence on environment, we will look at factors that may determine
the IMF: the mass of the pre-stellar core and the protostellar luminosity
(which has a significant contribution from accretion). Pre-stellar cores will
be extracted and characterized in terms of structure and mass. By combining
the protostellar SEDs from Spitzer with PACS photometry, particularly
70virgul mu m, better characterization of protostar bolometric luminosity and
temperature distributions can be produced and compared among the clouds
observed. With this data, we can examine how the core mass function and
protostellar luminosity function can vary w...ith density of young stars and cores
and with the local conditions of the molecular gas, and how these vary from
cloud to cloud.
Publication The SOFIA Massive (SOMA) Star Formation Survey. III. From Intermediate- to High-mass Protostars . Liu Mengyao et al. . The Astrophysical Journal . null . null . 2020ApJ...904...75L ,
The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope . Scicluna P. et al. . Monthly Notices of the Royal Astronomical Society . null . null . 2022MNRAS.512.1091S ,
Characterization of dense Planck clumps observed with Herschel and SCUBA-2 . Mannfors E. et al. . Astronomy and Astrophysics . null . null . 2021A&A...654A.123M ,
The SOFIA Massive (SOMA) Star Formation Survey. I. Overview and First Results . De Buizer James M. et al. . The Astrophysical Journal, Volume 843, Issue 1, article id. 33, 27 pp. (2017). . 843 . 10.3847\/1538-4357\/aa74c8 . 2017ApJ...843...33D ,
Detection of two power-law tails in the probability distribution functions of massive GMCs . Schneider N. et al. . Monthly Notices of the Royal Astronomical Society: Letters, Volume 453, p. L41-L45 . 453 . 10.1093\/mnrasl\/slv101 . 2015MNRAS.453L..41S ,
Star-Gas Surface Density Correlations in 12 Nearby Molecular Clouds. I. Data Collection and Star-sampled Analysis . Pokhrel Riwaj et al. . The Astrophysical Journal . null . null . 2020ApJ...896...60P ,
Clustering of low-mass stars around Herbig Be star IL Cep - evidence of .Rocket Effect. using Gaia EDR3 ? . Arun R. et al. . Monthly Notices of the Royal Astronomical Society . null . null . 2021MNRAS.507..267A ,
Instrument SPIRE\/PACS parallel_SpirePacsParallel_
Temporal Coverage 2013-02-17T02:05:57Z/2013-03-17T04:47:42Z
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/h®erschel/
Date Published 2013-09-16T17:42:38Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, gutermuth, r., 2013, OT1_rgutermu_1, SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-nbrzx4r