A dataset provided by the European Space Agency

Name OT2_pharve01_6
Title Disk Structure and Evolution Around Very Low Mass Stars
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342269684&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342269685&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342269737&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342269738&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342269739&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342269740&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342269741&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342269742&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342269743&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342269744&instrument_name=PACS&product_level=LEVEL0&compress=true

DOI 10.5270/esa-ids9anz
Author harvey, p.
Description We propose to observe the circumstellar disks around 28 very low mass stars that lie between the sub-stellar limit at 0.08 msun and 0.3-0.5 msun, the level where disks are bright enough to be readily detectable in the large, shallow Herschel surveys. The objects are located in 4 different star-forming regions that span a range of ages from roughly 1 - 3 Myr. This sample will provide the data necessary to link our understanding of disk evolution around solar-mass stars to those around sub-stellar objects, already well-represented by Herschel GT1 and OT1 programs. We will use proven disk modeling codes developed by team members and used extensively for modeling disks around stars and brown dwarfs. This approach has already worked well in our GT1 program on sub-stellar objects and in our first publication about its initial results.
Publication Herschel Photometry of Disks around Low-mass Stars in the R CrA Cloud . Harvey Paul M. et al. . The Astrophysical Journal, Volume 795, Issue 1, article id. 21, 6 pp. (2014). . 795 . 10.1088\/0004-637X\/795\/1\/21 . 2014ApJ...795...21H ,
Instrument PACS_PacsPhoto_largeScan
Temporal Coverage 2013-04-09T08:32:33Z/2013-04-09T21:27:21Z
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 ┬Ám range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/herschel/
Date Published 2013-10-09T21:01:11Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-10-09T21:01:11Z, OT2_pharve01_6, SPG v14.2.0. https://doi.org/10.5270/esa-ids9anz