A dataset provided by the European Space Agency

Name OT2_jrho01_4
Title Cold Dust in the Ejecta of Two Nearby Supernovae: Are supernovae dust producers in the early Universe?
URL

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DOI https://doi.org/10.5270/esa-9y2y1mg
Author rho, j.
Description Recent Herschel observations have detected up to 0.7 Msun of cold dust
surrounding SN 1987A . This discovery implies that supernovae could be
responsible for the large dust masses detected in high red-shift galaxies
and opens opportunities in the Herschel era for detecting and measuring
accurate cold dust masses in extra-galactic supernovae. One data point
from SN1987A is insufficient to resolve the fundamental question of the
origin of dust in early Universe, therefore we propose Herschel PACS and
SPIRE imaging observations of the two nearby supernovae SN 2004et and SN
2004dj. After SN 1987A, they are the closest well-known supernovae with
evidence of dust formation from Spitzer and other ground-based
observations. Our scientific goals are i) to detect far-infrared and submm
emission from supernovae, ii) to understand the spectral energy
distribution of the SNe for temperatures and dust composition, and iii) to
estimate freshly formed dust mass. These added observations are essential
to help determine if supernove are significant dust makers in the early
Universe.
Publication DustPedia: Multiwavelength photometry and imagery of 875 nearby galaxies in 42 ultraviolet-microwave bands . Clark C. J. R. et al. . Astronomy & Astrophysics, Volume 609, id.A37, 30 pp. . 609 . 10.1051\/0004-6361\/201731419 . 2018A&A...609A..37C ,
Probing the spectral shape of dust emission with the DustPedia galaxy sample . Nersesian Angelos et al. . Monthly Notices of the Royal Astronomical Society . null . null . 2021MNRAS.506.3986N ,
A nearby galaxy perspective on dust evolution. Scaling relations and constraints on the dust build-up in galaxies with the DustPedia and DGS samples . Galliano Frédéric et al. . Astronomy and Astrophysics . null . null . 2021A&A...649A..18G ,
Dust emissivity and absorption cross section in DustPedia late-type galaxies . Bianchi S. et al. . Astronomy and Astrophysics . null . null . 2019A&A...631A.102B ,
Fraction of bolometric luminosity absorbed by dust in DustPedia galaxies . Bianchi S. et al. . Astronomy & Astrophysics, Volume 620, id.A112, 21 pp. . 620 . 10.1051\/0004-6361\/201833699 . 2018A&A...620A.112B ,
UV to submillimetre luminosity functions of TNG50 galaxies . Trčka Ana et al. . Monthly Notices of the Royal Astronomical Society . null . null . 2022MNRAS.516.3728T ,
DustPedia: A Definitive Study of Cosmic Dust in the Local Universe . Davies J. I. et al. . Publications of the Astronomical Society of the Pacific, Volume 129, Issue 974, pp. 044102 (2017). . 129 . 10.1088\/1538-3873\/129\/974\/044102 . 2017PASP..129d4102D ,
Instrument PACS_PacsPhoto_largeScan, SPIRE_SpirePhoto_small
Temporal Coverage 2012-10-08T20:59:14Z/2013-03-01T08:32:52Z
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 2013-09-01T07:46:21Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, rho, j., 2013, OT2_jrho01_4, SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-9y2y1mg