IC 1816 | |
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![]() IC 1816 imaged by Dark Energy Survey. | |
Observation data (J2000 epoch) | |
Constellation | Fornax |
Right ascension | 02h 31m 50.97s [1] |
Declination | −36° 40′ 19.64″ [1] |
Redshift | 0.016945 ± 0.000020 [1] |
Heliocentric radial velocity | 5,080 km/s [1] |
Distance | 245 Mly |
Apparent magnitude (V) | 13.1 [2] |
Characteristics | |
Type | SB(r)ab pec? [1] |
Size | ~136,000 ly (41.7 kpc) (estimated) [1] |
Other designations | |
ESO 355-G025, MCG -06-06-011, AM 0229-365, IRAS 02297-3653, 6dF J0231510-364019, PGC 9634 [1] |
IC 1816 is a barred spiral galaxy located in the constellation of Fornax. The galaxy is located 245 million light-years from Earth and has a diameter of approximately 136,000 light-years across. [1] It was first discovered by Lewis Swift on 12 October 1896, who classified it as a small faint round object. [3]
IC 1816 is an isolated face-on spiral galaxy. [4] [5] It has three spiral arms with the northwest arm, the brightest and most detached. [5] Two of the arms are distinctive and seems to open up, as its spiral structure travels inwards. The galaxy also shows a prominent curved dust lane. [6] There is a clearly resolved ring and a smaller elongated structure interpreted as a nuclear bar. [5] An inner bar might be present given the observation of a small counter-rotation located from its nucleus although a nuclear disk is suggested. [7] The star formation rate for IC 1816 is estimated to be 0.74 Mʘ per year. [8]
The nucleus of IC 1816 is found active. It has been originally classified as a type 1 Seyfert galaxy [9] but later reclassified as a type 2 Seyfert galaxy due to it lacking broad emission lines. [10] The Seyfert spectrum of the galaxy is found extending as far as 3.4 arcseconds east from the nucleus. [11] A hydrogen alpha component is seen broadening, likely caused by the blending of nitrogen lines. [12]
IC 1816 has an extended narrow line region showing highly ionized gas, indicated by the presence of coronal line emission, with the region mainly centering in its star-forming ring. [13] Evidence showed the gas located in its nuclear region is mainly blueshifted with a peak velocity dispersion of 320 kilometers per seconds suggesting the active galactic nucleus of the galaxy is powered through outflows. [4]