Astronomy:PHL 293B

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PHL 293B
Observation data
ConstellationAquarius
Distance (comoving)22.6 million parsec
PHL 293B
Color image of PHL 293B.tif
Hubble Space Telescope image of PHL 293B; the purported luminous blue variable is located near the core of the galaxy
Credit: NASA, ESA/Hubble, J. Andrews (U. Arizona)
Observation data
Equinox J2000.0]] (ICRS)
Constellation Aquarius
Right ascension  22h 28.1m[1]
Declination −0° 22′[1]
Characteristics
Evolutionary stage Luminous blue variable?
Astrometry
Radial velocity (Rv)(of galaxy) 1,606[2] km/s
Distance22,600,000[3] pc
Details
Radius1,348–1,463[4] R
Luminosity2,500,000–3,500,000[4] L
Temperature6,000–6,800[4] K
Other designations
Kinman's dwarf,[5] SDSS J2230–0006,[6] SDSS J223036.79-000636.9, A2228-00[5]
Database references
SIMBADPHL 293B
PHL 293 (Simbad mistakenly showing results for PHL 293B)

PHL 293B, also known as Kinman's dwarf, is a low-metallicity blue compact dwarf galaxy about 22.6 Mpc from the Earth in the constellation Aquarius.[3]

It had a very likely associated, notable, blue-light, long-lived star with constant outbursts or a large supernova observed to have faded and which then disappeared. Although this bright visible jet-producing object responsible for broad hydrogen emission lines with P Cygni profiles was widely considered to be a luminous blue variable ejecting matter, other studies posited the mentioned, competing, explanations for the bright light source within.

Observation history

PHL 293 was first listed as entry 293 in a catalogue of faint blue stars published by Guillermo Haro and Willem Jacob Luyten in 1962.[7] In 1965, Thomas Kinman observed two faint possible companions to it, about 1 away, which he dubbed A and B. HL 293B, sometimes called Kinman's Dwarf, was noted to be an extragalactic, nonstellar object, with a jet, approximately 22.6 Mpc away from Earth.[3][5] The acronym PHL has since been applied to distinguish it from other HL catalogues; it is most commonly referred to by astronomers as PHL 293B.[1] The galaxy was identified as a blue compact dwarf, a type of small irregular galaxy undergoing a strong burst of star formation.[6]

The spectrum of PHL 293B is unusual both for its low metallicity and for broad hydrogen emission lines with P Cygni profiles. These are interpreted as being from a large luminous blue variable star in the galaxy. The star is believed to have been undergoing an outburst during previous observations,[6] an interpretation is disputed by some publications.[citation needed] An alternative explanation would be a long-lived type IIn supernova, similar to the transient event of SDSS1133.[8] These emission features in the spectrum of the galaxy faded during 2019 and by the end of the year had disappeared (at least visibly), likely due to the disappearance of a bright star of the galaxy.[4]

See also

References

  1. 1.0 1.1 1.2 French, H. B. (1980). "Galaxies with the spectra of giant H II regions". The Astrophysical Journal 240: 41. doi:10.1086/158205. Bibcode1980ApJ...240...41F. 
  2. Guseva, N. G.; Papaderos, P.; Meyer, H. T.; Izotov, Y. I.; Fricke, K. J. (2009). "An investigation of the luminosity-metallicity relation for a large sample of low-metallicity emission-line galaxies". Astronomy & Astrophysics 505 (1): 63–72. doi:10.1051/0004-6361/200912414. Bibcode2009A&A...505...63G. 
  3. 3.0 3.1 3.2 Kinman, T. D. (1965). "The Nature of the Fainter Haro-Luyten Objects". The Astrophysical Journal 142: 1241. doi:10.1086/148392. Bibcode1965ApJ...142.1241K. 
  4. 4.0 4.1 4.2 4.3 Allan, Andrew P.; Groh, Jose H.; Mehner, Andrea; Smith, Nathan; Boian, Ioana; Farrell, Eoin J.; Andrews, Jennifer E. (2020). "The possible disappearance of a massive star in the low-metallicity galaxy PHL 293B". Monthly Notices of the Royal Astronomical Society 496 (2): 1902. doi:10.1093/mnras/staa1629. Bibcode2020MNRAS.496.1902A. 
  5. 5.0 5.1 5.2 Terlevich, Roberto; Terlevich, Elena; Bosch, Guillermo; Díaz, Ángeles; Hägele, Guillermo; Cardaci, Mónica; Firpo, Verónica (2014). "High-velocity blueshifted Fe ii absorption in the dwarf star-forming galaxy PHL 293B: Evidence for a wind driven supershell?". Monthly Notices of the Royal Astronomical Society 445 (2): 1449–1461. doi:10.1093/mnras/stu1806. Bibcode2014MNRAS.445.1449T. 
  6. 6.0 6.1 6.2 Izotov, Yuri I.; Thuan, Trinh X. (2009). "Luminous Blue Variable Stars in the two Extremely Metal-Deficient Blue Compact Dwarf Galaxies DDO 68 and PHL 293B". The Astrophysical Journal 690 (2): 1797–1806. doi:10.1088/0004-637X/690/2/1797. Bibcode2009ApJ...690.1797I. 
  7. Haro, G.; Luyten, W. J. (1962). "Faint Blue Stars in the Region near the South Galactic Pole". Boletín de los Observatorios de Tonantzintla y Tacubaya 3: 37. Bibcode1962BOTT....3...37H. 
  8. Burke, Colin J.; Baldassare, Vivienne F.; Liu, Xin; Foley, Ryan J.; Shen, Yue; Palmese, Antonella; Guo, Hengxiao; Herner, Kenneth et al. (2020). "The Curious Case of PHL 293B: A Long-lived Transient in a Metal-poor Blue Compact Dwarf Galaxy". The Astrophysical Journal 894 (1): L5. doi:10.3847/2041-8213/ab88de. Bibcode2020ApJ...894L...5B.