Zobrazeno 1 - 10
of 19
pro vyhledávání: '"Arkaprabha Sarangi"'
Autor:
Arkaprabha Sarangi
Publikováno v:
Sarangi, A 2022, ' Formation, distribution, and IR emission of dust in the clumpy ejecta of Type II-P core-collapse supernovae, in isotropic and anisotropic scenarios ', Astronomy & Astrophysics, vol. 668, A57 . https://doi.org/10.1051/0004-6361/202244391
Large discrepancies are found between observational estimates and theoretical predictions when exploring the characteristics of dust formed in the ejecta of core-collapse supernovae. We revisit the scenario of dust production in typical supernova eje
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6bdcfb78582de3b15c5a600ffa734111
Autor:
Arkaprabha Sarangi, Jonathan D. Slavin
Publikováno v:
Sarangi, A & Slavin, J D 2022, ' Dust Production in a Thin Dense Shell in Supernovae with Early Circumstellar Interactions ', Astrophysical Journal, vol. 933, no. 1, 89 . https://doi.org/10.3847/1538-4357/ac713d
In supernovae (SNe), where the light curves show evidence of strong and early interaction between the ejecta and the circumstellar matter (CSM), the formation of new dust is estimated to take place in a dense shell of gas between the forward (FS) and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d7bfe9c43472211c793165f4ee6891e6
https://doi.org/10.3847/1538-4357/ac713d
https://doi.org/10.3847/1538-4357/ac713d
Autor:
Timothy R. Kallman, Arkaprabha Sarangi, Ori D. Fox, Richard G. Arendt, Eli Dwek, Demos Kazanas
Publikováno v:
The Astrophysical Journal. 917:84
SN 2010jl is a Type IIn core collapse supernova whose radiative output is powered by the interaction of the SN shock wave with its surrounding dense circumstellar medium (CSM). After day ~60, its light curve developed a NIR excess emission from dust.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::52006551e70fd7d340abaf62d07eb669
https://doi.org/10.3847/1538-4357/ac09ea
https://doi.org/10.3847/1538-4357/ac09ea
Infrared (IR) observations of core collapse supernovae (CCSNe) have been used to infer the mass of dust that has formed in their ejecta. A plot of inferred dust masses versus supernova (SN) ages shows a trend of increasing dust mass with time, spanni
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b317f9b2a972f80ff9ff169f64404ead
We model the fluxes in the infrared and submillimeter domain using the dust chemical composition and mass derived from the physico-chemical model of a Type II-P supernova ejecta with stellar progenitor of 19 M⊙. Our results highlight that the dust
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5b5d7f89bccd74e680cf63d1822a2725
http://doc.rero.ch/record/300683/files/S1743921313009988.pdf
http://doc.rero.ch/record/300683/files/S1743921313009988.pdf
Publikováno v:
The Astrophysical Journal. 885:126
Infrared observations of active galactic nucleus (AGN) reveal emission from the putative dusty circumnuclear 'torus' invoked by AGN unification, that is heated up by radiation from the central accreting black hole (BH). The strong 9.7 and 18 micron s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::031fb33fd1d49320aa95475e6d1a3f42
https://doi.org/10.3847/1538-4357/ab46a9
https://doi.org/10.3847/1538-4357/ab46a9
Publikováno v:
Proceedings of the International Astronomical Union. 9:151-154
We study the formation of molecules and dust clusters in the ejecta of solar metallicity, Type II-P supernovae using a chemical kinetic approach and follow the evolution of molecules and small dust cluster masses from day 100 to day 1500 after explos
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::66ecec837250d87d439bbbf89ba139cc
https://doi.org/10.1017/s1743921313009381
https://doi.org/10.1017/s1743921313009381
Publikováno v:
The Astrophysical Journal. 859:66
The light curves of Type IIn supernovae are dominated by the radiative energy released through the interaction of the supernova shockwaves with their dense circumstellar medium (CSM). The ultraluminous Type IIn supernova SN 2010jl exhibits an infrare
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::770d212232a8a449ad433f9ee9eec0c6
https://doi.org/10.3847/1538-4357/aabfc3
https://doi.org/10.3847/1538-4357/aabfc3
Aims: We study the production of dust in Type II-P supernova by coupling the gas-phase chemistry to the dust nucleation and condensation phases. We consider two supernova progenitor masses with homogeneous and clumpy ejecta to assess the chemical typ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d4a7a36f181c54050d29ffacc9d01f5f
http://arxiv.org/abs/1412.5522
http://arxiv.org/abs/1412.5522
Publikováno v:
Proceedings of The Life Cycle of Dust in the Universe: Observations, Theory, and Laboratory Experiments — PoS(LCDU2013).
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::86c708b10175c06fa43ffed69fa85afc
https://doi.org/10.22323/1.207.0091
https://doi.org/10.22323/1.207.0091