PHL 293B

PHL 293B
Hubble Space Telescope image of PHL 293B; the purported luminous blue variable is located near the core of the galaxy
Observation data (J2000 epoch)
ConstellationAquarius
Right ascension22h 30m 36.8s
Declination−00° 06′ 37″
Redshift0.0051
Heliocentric radial velocity1,606 km/s
Galactocentric velocity1,723±10 km/s
Distance75.51 ± 8.072 Mly (23.150 ± 2.475 Mpc)
Apparent magnitude (V)16.87
Apparent magnitude (B)17.35
Characteristics
Typecompact Im? HII
Size5,450 ly × 4,960 ly
(1.67 kpc × 1.52 kpc)
(diameter; 25.0 B-mag arcsec−2)
Apparent size (V)0.24 × 0.20
Other designations
Kinman's Dwarf, PGC 69018
PHL 293B star
Observation data
Epoch J1950      Equinox J1950
Constellation Aquarius
Right ascension 22h 28.1m
Declination −0° 22′
Characteristics
Evolutionary stage Luminous blue variable?
Astrometry
Radial velocity (Rv)(of galaxy) 1,606 km/s
Distance23,150,000±2,475,000 pc
Details
Radius1,348–1,463 R
Luminosity2,500,000–3,500,000 L
Temperature6,000–6,800 K
Other designations
SDSS J2230–0006, SDSS J223036.79-000636.9, A2228-00
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 23.15 megaparsecs (75.51 million light-years) from the Earth in the constellation Aquarius.

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.