Supernova 2014C: ongoing interaction with extended circumstellar material with silicate dust

@article{Tinyanont2019Supernova2O,
  title={Supernova 2014C: ongoing interaction with extended circumstellar material with silicate dust},
  author={S. Tinyanont and R. Lau and M. Kasliwal and K. Maeda and N. Smith and O. D. Fox and R. Gehrz and K. De and J. Jencson and J. Bally and F. Masci},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2019}
}
Supernova (SN) 2014C is a unique explosion where a seemingly typical hydrogen-poor stripped envelope SN started to interact with a dense, hydrogen-rich circumstellar medium (CSM) a few months after the explosion. The delayed interaction suggests a detached CSM shell, unlike in a typical SN IIn where the CSM is much closer and the interaction commences earlier post-explosion; indicating a different mass loss history. We present near- to mid-infrared observations of SN 2014C from 1-5 years after… Expand
3 Citations

References

SHOWING 1-10 OF 73 REFERENCES
Stripped-envelope supernova SN 2004dk is now interacting with hydrogen-rich circumstellar material
  • 9
  • PDF
Metamorphosis of SN 2014C: Delayed Interaction Between a Hydrogen Poor Core-collapse Supernova and a Nearby Circumstellar Shell
  • 56
  • Highly Influential
  • PDF
Ejection of the Massive Hydrogen-rich Envelope Timed with the Collapse of the Stripped SN 2014C.
  • 66
  • Highly Influential
  • PDF
SN 2014C: VLBI Images of a Supernova Interacting with a Circumstellar Shell
  • 6
  • Highly Influential
  • PDF
The peculiar mass-loss history of SN 2014C as revealed through AMI radio observations
  • 13
  • Highly Influential
  • PDF
LATE-TIME CIRCUMSTELLAR INTERACTION IN A SPITZER SELECTED SAMPLE OF TYPE IIn SUPERNOVAE
  • 50
  • PDF
LATE-TIME DUST EMISSION FROM THE TYPE IIn SUPERNOVA 1995N
  • 7
  • PDF
Interacting Supernovae: Types IIn and Ibn
  • 58
  • PDF
Late Emission from the Type Ib/c SN 2001em: Overtaking the Hydrogen Envelope
  • 53
  • PDF
...
1
2
3
4
5
...