Near-Infrared observations of the type Ib Supernova SN2006jc: evidence of interactions with dust
arXiv:0712.3855 · doi:10.1086/590051
Abstract
In the framework of a program for the monitoring of Supernovae in the Near-Infrared (NIR) carried out by the Teramo, Rome and Pulkovo observatories with the AZT-24 telescope, we observed the Supernova SN2006jc in the J,H,K photometric bands during a period of 7 months, starting ~36 days after its discovery. Our observations evidence a NIR re-brightening, peaking ~70 days after discovery, along with a reddening of H-K and J-H colors until 120 days from discovery. After that date, J-H seems to evolve towards bluer colors. Our data, complemented by IR, optical, UV and X-ray observations found in the literature, show that the re-brightening is produced by hot dust surrounding the supernova, formed in the interaction of the ejecta with dense circumstellar matter.
22 pages, 5 figures, submitted to ApJ
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- The Peculiar Type Ib Supernova 2006jc: A WCO Wolf-Rayet Star Explosion
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- Optical photometry and spectroscopy of the type Ibn supernova SN 2006jc until the onset of dust formation
- High-resolution spectroscopy of SN 2017hcc and its blueshifted line profiles from post-shock dust formation
- Near-Infrared and Optical Observations of Type Ic SN 2021krf: Luminous Late-time Emission and Dust Formation
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- Massive stars exploding in a He-rich circumstellar medium X. Flash spectral features in the Type Ibn SN 2019cj and observations of SN 2018jmt