UGC 711
UGC 711
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UGC 711

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UGC 711
UGC 711 imaged by SDSS. The star to the left of the galaxy is TYC 19-146-2
Observation data (J2000 epoch)
ConstellationCetus
Right ascension01h 08m 36.90s
Declination+01° 38′ 30.0″
Redshift0.006611
Heliocentric radial velocity1,982 km/s
Distance77 Mly (23.6 Mpc)
Apparent magnitude (V)0.069
Apparent magnitude (B)0.092
Surface brightness14.39
Characteristics
TypeSB (s)d?, sp
Apparent size (V)4.65' x 0.30'
Notable featuresSuperthin spiral galaxy
Other designations
PGC 4063, FGC 0124, RFGC 0255, MCG +00-04-008, CGCG 385-005

UGC 711 is a spiral galaxy located in the constellation of Cetus. Estimated to be located 77 million light-years from Earth,[1] the galaxy's luminosity class is IV and it has a HI line width region.[clarification needed][2] It belongs to the equatorial region of Eridanus Void with an arcsec approximation of ≈ 250.[clarification needed][3]

Morphology

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UGC 711 is considered a low-surface brightness galaxy (LSB)[4] with a diffuse stellar disk.[5][6]

With a surface brightness measurement found ~1 magnitude less illuminated compared to μ B,0 = 21.65 mag arcsec−2 according to K.C. Freeman,[7] UGC 711 is one of best studied superthin galaxies defined by its atypical classification when seen edge-on.[8][9][10] It has a flat structure with only a diameter estimating to be a = 40 arcsecs but has a major-to-minor axis ratio wider than 7 arcsecs.[11]

The rotational velocity of UGC 711 is said to be only Vcirc = 92 km s−1 according to measurements from Hyperleda.[12]

References

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