Dust in Supernovae and Supernova Remnants I: Formation Scenarios
Supernovae are considered as prime sources of dust in space. Observations of local supernovae over the past couple of decades have detected the presence of dust in supernova ejecta. The reddening of the high redshift quasars also indicate the presence of large masses of dust in early galaxies. Consi...
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| Veröffentlicht in: | Space science reviews 2018-04, Vol.214 (3), p.1-48 |
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| creator | Sarangi, A. Matsuura, M. Micelotta, E. R. |
| description | Supernovae are considered as prime sources of dust in space. Observations of local supernovae over the past couple of decades have detected the presence of dust in supernova ejecta. The reddening of the high redshift quasars also indicate the presence of large masses of dust in early galaxies. Considering the top heavy IMF in the early galaxies, supernovae are assumed to be the major contributor to these large amounts of dust. However, the composition and morphology of dust grains formed in a supernova ejecta is yet to be understood with clarity. Moreover, the dust masses inferred from observations in mid-infrared and submillimeter wavelength regimes differ by two orders of magnitude or more. Therefore, the mechanism responsible for the synthesis of molecules and dust in such environments plays a crucial role in studying the evolution of cosmic dust in galaxies. This review summarises our current knowledge of dust formation in supernova ejecta and tries to quantify the role of supernovae as dust producers in a galaxy. |
| doi_str_mv | 10.1007/s11214-018-0492-7 |
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Observations of local supernovae over the past couple of decades have detected the presence of dust in supernova ejecta. The reddening of the high redshift quasars also indicate the presence of large masses of dust in early galaxies. Considering the top heavy IMF in the early galaxies, supernovae are assumed to be the major contributor to these large amounts of dust. However, the composition and morphology of dust grains formed in a supernova ejecta is yet to be understood with clarity. Moreover, the dust masses inferred from observations in mid-infrared and submillimeter wavelength regimes differ by two orders of magnitude or more. Therefore, the mechanism responsible for the synthesis of molecules and dust in such environments plays a crucial role in studying the evolution of cosmic dust in galaxies. This review summarises our current knowledge of dust formation in supernova ejecta and tries to quantify the role of supernovae as dust producers in a galaxy.</description><subject>Aerospace Technology and Astronautics</subject><subject>Astrophysics and Astroparticles</subject><subject>Chemical synthesis</subject><subject>Cosmic dust</subject><subject>Dust</subject><subject>Ejecta</subject><subject>Ejection</subject><subject>Evolution</subject><subject>Galactic evolution</subject><subject>Galaxies</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Planetology</subject><subject>Quasars</subject><subject>Red shift</subject><subject>Space Exploration and Astronautics</subject><subject>Space Sciences (including Extraterrestrial Physics</subject><subject>Supernova</subject><subject>Supernova remnants</subject><subject>Supernovae</subject><issn>0038-6308</issn><issn>1572-9672</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><sourceid>C6C</sourceid><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GNUQQ</sourceid><recordid>eNpFkE9LxDAQxYMoWFc_gLeC5-hkkiatJ2Xd1YUFwT_nkLZT6eKmNWn9_LassKfHwO_N4z3GrgXcCgBzF4VAoTiInIMqkJsTlojMIC-0wVOWAMicawn5ObuIcQcwu0zCHp7GOKStT9_HnoLvfh2lztfHM32jvXd-iOnmPl13Ye-GtpvwirwLbRcv2VnjviNd_euCfa5XH8sXvn193iwft7wXmR54IUtTZBmJxqFqEMqyKI1CRRoJpJGkVE2UVaRdpWuFLs-pwjorZQWiFo1csJvD3z50PyPFwe66Mfgp0uLUutCYGzNReKBiH1r_ReFICbBzZ3tYyk4eOy9ljfwDbatbUA</recordid><startdate>20180401</startdate><enddate>20180401</enddate><creator>Sarangi, A.</creator><creator>Matsuura, M.</creator><creator>Micelotta, E. 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| subjects | Aerospace Technology and Astronautics Astrophysics and Astroparticles Chemical synthesis Cosmic dust Dust Ejecta Ejection Evolution Galactic evolution Galaxies Physics Physics and Astronomy Planetology Quasars Red shift Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Supernova Supernova remnants Supernovae |
| title | Dust in Supernovae and Supernova Remnants I: Formation Scenarios |
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