A dataset provided by the European Space Agency

Name GT1_jblommae_1
Title Forsterite dust in the circumstellar environment of evolved stars
URL

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http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342229802&instrument_name=PACS&product_level=LEVEL0&compress=true

DOI 10.5270/esa-lbobehb
Author blommaert, j.
Description PACS range spectroscopy will be performed around the 69 micron forsterite dust feature of evolved stars. With the spectral resolution and sensitivity of PACS we will be able to fit the profile of the forsterite feature which is very sensitive to temperature. By studying the forsterite feature in a wide range of evolved stars and from different populations (including Galactic Bulge and LMC) we want to determine the role of forsterite in the dust formation in the circumstellar environments.
Publication THROES: a caTalogue of HeRschel Observations of Evolved Stars. I. PACS range spectroscopy . Ramos-Medina J. et al. . Astronomy & Astrophysics, Volume 611, id.A41, 38 pp. . 611 . 10.1051\/0004-6361\/201731940 . 2018A&A...611A..41R ,
Herschel-PACS observations of the 69 μm band of crystalline olivine around evolved stars . Blommaert J. A. D. L. et al. . Astronomy & Astrophysics, Volume 565, id.A109, 16 pp. . 565 . 10.1051\/0004-6361\/201322554 . 2014A&A...565A.109B ,
Instrument PACS_PacsRangeSpec_point
Temporal Coverage 2010-10-23T15:44:01Z/2011-09-27T08:02:59Z
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 2012-03-27T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-03-27T00:00:00Z, GT1_jblommae_1, SPG v14.2.0. https://doi.org/10.5270/esa-lbobehb