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Type Iax supernova

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A type Iax supernova is a rare subtype of type Ia supernova, which leaves behind a remnant star, known as zombie star, rather than completely dispersing the white dwarf.[1][2][3][4][5] Type Iax supernovae are similar to type Ia, but have a lower ejection velocity and lower luminosity.[6] Type Iax supernovae may occur at a rate between 5 and 30 percent of the Ia supernova rate. As of October 2014, thirty supernovae had been identified in this category.[7]

In a binary system consisting of a white dwarf and a companion star, the white dwarf strips away material from its companion. Normally the white dwarf would eventually reach a critical mass, and fusion reactions would make it explode and completely dissipate it, but in a Type Iax supernova, only a part of the dwarf's mass is lost.[8]

The two inset images show before-and-after images captured by NASA's Hubble Space Telescope of Supernova 2012Z in the spiral galaxy NGC 1309. The white X at the top of the main image marks the location of the supernova in the galaxy.

Candidate observed instances

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Supernova SN 2012Z in the galaxy NGC 1309 is thought to be of type Iax, and was discovered by Brad Cenko, Weidong Li, and Alex Filippenko using the Katzman Automatic Imaging Telescope on 2012 January 29.15 UT as part of a supernova search at Lick Observatory.

The proposed formation scenario for SN 2012Z is that the original system at the heart of the supernova was a binary pair of large, but otherwise ordinary main sequence stars. The more massive of the binary stars lost substantial amounts of its hydrogen and helium to its smaller companion, and became a white dwarf. The newly engorged companion star then evolved into an enlarged stage, whose outer layers engulfed the white dwarf. The outer hydrogen layers of the overlapping stars were then ejected, leaving behind a still-active helium core and the white dwarf. In turn, the white dwarf drained back some matter from the remaining companion star, until the white dwarf became so unstable that it exploded as a supernova, with the former helium core left behind as a remnant zombie star.[3]

There were images of the area from before the supernova, allowing before and after images, and the process of the supernova to be studied. To test the zombie star hypothesis, the area was observed again a few years after the event. The authors found that the decline of the light curve was consistent with the existence of a radioactively-heated bound remnant, but that it was difficult to come up with a model that could explain the whole light curve.[9]

This discovery is a milestone in a decades long search by astronomers for such an occurrence; the observation of SN 2012Z was the first time astrophysicists were able to identify a star system that later went to a supernova of this type.[8]

SN 2008ha may be a type Iax supernova, but significantly weaker than SN 2012Z.[3]

On 13 September 2024, BlackGEM discovered an astronomical transient, designated SN 2024vjm, in NGC 6744.[10] After initial spectral analysis the star was classified as a peculiar nova, but further observations showed the object to be a faint type Iax supernova, likely the closest known of this type.[11][12][13]

SN 1181

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Pa 30 and the central star IRAS 00500+6713, which is a zombie star
Main articles: SN 1181 and IRAS 00500+6713

SN 1181 was observed by Chinese and Japanese astronomers in 1181 AD. The amateur astronomer Dana Patchick first discovered the nebula Pa 30 with WISE. The nebula Pa 30 was connected to SN 1181 by astronomers and has the central star IRAS 00500+6713. The central star is an oxygen-rich Wolf–Rayet star and is the result of a merger of a CO (carbon-oxygen) white dwarf and an ONe (oxygen–neon–magnesium) white dwarf in a type Iax supernova. This makes IRAS 00500+6713 a confirmed zombie star. Pa 30 and IRAS 00500+6713 is the only known remnant of a type Iax in the Milky Way.[14][15][16]

References

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  1. ^ Hubbard, Amy (6 August 2014). "Hubble sees 'zombie star' lurking in space: What it is, why it matters". Los Angeles Times. Retrieved 30 October 2014.
  2. ^ "Hubble discovers 'zombie star' haunting the universe". CNET. Retrieved 30 October 2014.
  3. ^ a b c Weaver, Donna; Villard, Ray (6 August 2014). "NASA's Hubble Finds Supernova Star System Linked to Potential "Zombie Star"". HubbleSite – NewsCenter. NASA. Retrieved 30 October 2014.
  4. ^ "Zombie star: Hubble spots star SN 2012Z living after supernova". Slate Magazine (Video). 12 August 2014. Retrieved 30 October 2014.
  5. ^ Hauk, Alexis (6 August 2014). "Hubble Finds Supernova Star System Linked to Potential "Zombie Star"". Time Magazine. Retrieved 30 October 2014.
  6. ^ McCully, Curtis; Jha, Saurabh W.; Foley, Ryan J.; Bildsten, Lars; Fong, Wen-fai; Kirshner, Robert P.; Marion, G. H.; Riess, Adam G.; Stritzinger, Maximilian D. (7 August 2014). "A luminous, blue progenitor system for the Type Iax supernova 2012Z". Nature. 512 (512): 54–56. arXiv:1408.1089. Bibcode:2014Natur.512...54M. doi:10.1038/nature13615. PMID 25100479. S2CID 4464556.
  7. ^ Feltman, Rachel. "Astronomers may have found a new zombie star". Washington Post. Archived from the original on 30 October 2014. Retrieved 30 October 2014.
  8. ^ a b Choi, Charles Quixote (6 August 2014). "Supernovas Might Create Weird 'Zombie Stars'". Space.com. Retrieved 30 October 2014.
  9. ^ Curtis McCully; Saurabh W. Jha; Richard A. Scalzo; D. Andrew Howell; Ryan J. Foley; Yaotian Zeng; Zheng-Wei Liu; Griffin Hosseinzadeh; Lars Bildsten; Adam G. Riess; Robert P. Kirshner; G. H. Marion; Yssavo Camacho-Neves (2022). "Still Brighter than Pre-explosion, SN 2012Z Did Not Disappear: Comparing Hubble Space Telescope Observations a Decade Apart". The Astrophysical Journal. 925 (2): 138. arXiv:2106.04602. Bibcode:2022ApJ...925..138M. doi:10.3847/1538-4357/ac3bbd.
  10. ^ "Discovery certificate for object 2024vjm". Transient Name Server. IAU. Retrieved 15 September 2024.
  11. ^ "SN 2024vjm". Transient Name Server. IAU. Retrieved 15 September 2024.
  12. ^ "AstroNote 2024-258". Transient Name Server. IAU. Retrieved 15 September 2024.
  13. ^ "AstroNote 2024-265". Transient Name Server. IAU. Retrieved 20 September 2024.
  14. ^ Ritter, Andreas; Parker, Quentin A.; Lykou, Foteini; Zijlstra, Albert A.; Guerrero, Martin A.; Le Du, Pascal (7 Nov 2023). "From an amateur PN candidate to the Rosetta Stone of SN Iax research". IAU 384 Conference Proceedings: 6. arXiv:2311.03700. Bibcode:2023arXiv231103700R.
  15. ^ Fesen, Robert A.; Schaefer, Bradley E.; Patchick, Dana (2023-03-01). "Discovery of an Exceptional Optical Nebulosity in the Suspected Galactic SN Iax Remnant Pa 30 Linked to the Historical Guest Star of 1181 CE". The Astrophysical Journal Letters. 945 (1): L4. arXiv:2301.04809. Bibcode:2023ApJ...945L...4F. doi:10.3847/2041-8213/acbb67. ISSN 2041-8205.
  16. ^ Ko, Takatoshi; Suzuki, Hiromasa; Kashiyama, Kazumi; Uchida, Hiroyuki; Tanaka, Takaaki; Tsuna, Daichi; Fujisawa, Kotaro; Bamba, Aya; Shigeyama, Toshikazu (2024). "A Dynamical Model for IRAS 00500+6713: The Remnant of a Type Iax Supernova SN 1181 Hosting a Double Degenerate Merger Product WD J005311". The Astrophysical Journal. 969 (2): 116. arXiv:2304.14669. Bibcode:2024ApJ...969..116K. doi:10.3847/1538-4357/ad4d99.
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