NGC 7090 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Indus |
Right ascension | 21h 36m 28.865s[3] |
Declination | −54° 33′ 26.35″[3] |
Redshift | 0.002859±0.000020[4] |
Heliocentric radial velocity | 846 km/s[5] |
Distance | 31.0 Mly (9.5 Mpc)[6] |
Apparent magnitude (V) | 10.51[7] |
Characteristics | |
Type | Scd[8] |
Mass | Stellar: 5.47×109[6] M☉ |
Other designations | |
IRAS 21329-5446, 2MASX J21362886-5433263, NGC 7090, LEDA 67045[7] |
NGC 7090 is a spiral galaxy[8] in the southern constellation of Indus located about 31 million light-years away.[6] English astronomer John Herschel first observed this galaxy on 4 October 1834.[1][2]
The morphological class of NGC 7090 is Scd,[8] indicating it is a spiral with loosely-wound and somewhat disorganized arms. The galactic plane is inclined at an angle of 89° to the line of sight from the Earth,[8] giving it an edge-on view. The combined mass of the stars in this galaxy is 5.5 billion times the mass of the Sun (M☉), while the star formation rate is ~0.5 M☉·yr−1.[6] As a result of star formation, the diffuse ionized gas in the galaxy has a complex organization, showing filaments, bubbles, and super-shells.[9]
Three transient ultraluminous X-ray sources have been detected in NGC 7090.[10][11]
Hubble2012
was invoked but never defined (see the help page).esa/hubble
was invoked but never defined (see the help page).Skrutskie_et_al_2006
was invoked but never defined (see the help page).de_vaucoulerus_et_al_1991
was invoked but never defined (see the help page).Tully_et_al_2016
was invoked but never defined (see the help page).Lianou_et_al_2019
was invoked but never defined (see the help page).simbad
was invoked but never defined (see the help page).Heesen_et_al_2016
was invoked but never defined (see the help page).Rossa_et_al_2012
was invoked but never defined (see the help page).Liu_et_al_2019
was invoked but never defined (see the help page).Walton_et_al_2021
was invoked but never defined (see the help page).