| NGC 959 | |
|---|---|
 | |
| Observation data (J2000 epoch) | |
| Constellation | Triangulum |
| Right ascension | 02h 32m 23.923s [1] |
| Declination | +35° 29′ 40.46″ [1] |
| Heliocentric radial velocity | 596 km/s [2] |
| Distance | 36 Mly (11.0 Mpc) [2] [3] |
| Group or cluster | NGC 1023 Group [4] |
| Apparent magnitude (V) | 12.38±0.14 [3] |
| Apparent magnitude (B) | 12.95±0.14 [3] |
| Characteristics | |
| Type | Sdm: [3] or SBcd [5] |
| Mass | 6.3×108 [6] (stellar) M☉ |
| Size | 21.8 kly (6.69 kpc) [7] |
| Apparent size (V) | 2′.3 × 1′.4 [3] (D25) |
| Other designations | |
| IRAS 02293+3516, NGC 959, UGC 2002, LEDA 9665, MCG +06-06-051, PGC 9665 [8] [9] | |
NGC 959 is a spiral galaxy in the northern constellation of Triangulum. [10] It was discovered on November 9, 1876, by French astronomer Édouard Stephan. [9] This galaxy is located at a distance of 36 million light years and is receding with a heliocentric radial velocity of 596 km/s. [2] It is a member of the NGC 1023 Group of galaxies. [4]
The morphological class of this galaxy is Sdm:, [3] indicating it is a spiral (S) with disorganized, irregular arms and no central bulge (dm). The ':' suffix indicates some uncertainty about the classification. It has a visual magnitude of 12.4. [3] The galactic plane is inclined at an angle of 50° to the line of sight from the Earth, [11] giving it an elliptical profile with the major axis aligned along a position angle of 65°. The size of the D25 ellipse (where the brightness of the galaxy drops to magnitude 25) is 2.3 × 1.4 arcminutes. [3]
When images of NGC 959 are corrected for the effects of extinction from dust, a central bar feature can be discerned. The galaxy then shows a non-negligible bulge or central condensation, and may instead have a morphological type of SBcd. [5] It displays a cuspy central density profile and bulge-like monotonic decrease in ellipticity toward the core. [6]
- ^ a b Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv: 1804.09365. Bibcode: 2018A&A...616A...1G. doi: 10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ a b c Tully, R. Brent; et al. (August 2016), "Cosmicflows-3", The Astronomical Journal, 152 (2): 21, arXiv: 1605.01765, Bibcode: 2016AJ....152...50T, doi: 10.3847/0004-6256/152/2/50, S2CID 250737862, 50.
- ^ a b c d e f g h Gil de Paz, Armando; et al. (December 2007), "The GALEX Ultraviolet Atlas of Nearby Galaxies", The Astrophysical Journal Supplement Series, 173 (2): 185–255, arXiv: astro-ph/0606440, Bibcode: 2007ApJS..173..185G, doi: 10.1086/516636, S2CID 119085482.
- ^ a b Trentham, Neil; Tully, R. Brent (September 2009), "Dwarf galaxies in the NGC 1023 Group", Monthly Notices of the Royal Astronomical Society, 398 (2): 722–734, arXiv: 0906.2540, Bibcode: 2009MNRAS.398..722T, doi: 10.1111/j.1365-2966.2009.15189.x, S2CID 18442520.
- ^ a b Tamura, K.; et al. (June 2010), "Lifting the Veil of Dust from NGC 0959: The Importance of a Pixel-based Two-dimensional Extinction Correction", The Astronomical Journal, 139 (6): 2557–2565, arXiv: 1004.3575, Bibcode: 2010AJ....139.2557T, doi: 10.1088/0004-6256/139/6/2557, S2CID 119274723.
- ^ a b Relatores, Nicole C.; et al. (December 2019), "The Dark Matter Distributions in Low-mass Disk Galaxies. II. The Inner Density Profiles", The Astrophysical Journal, 887 (1): 23, arXiv: 1911.05836, Bibcode: 2019ApJ...887...94R, doi: 10.3847/1538-4357/ab5305, S2CID 208006358, 94.
- ^ Truong, Phuongmai N.; et al. (July 2017), "High-resolution Velocity Fields of Low-mass Disk Galaxies. I. CO Observations", The Astrophysical Journal, 843 (1): 15, Bibcode: 2017ApJ...843...37T, doi: 10.3847/1538-4357/aa76eb, S2CID 23645373, 37.
-
^
"NGC 959".
SIMBAD.
Centre de données astronomiques de Strasbourg. Retrieved 2022-01-18.
{{ cite web}}: CS1 maint: postscript ( link) - ^ a b Seligman, Courtney, "NGC Objects: NGC 950 - 999", Celestial Atlas, retrieved 2022-01-18.
- ^ Aranda, Ted (2011), 3,000 Deep-Sky Objects, An Annotated Catalogue, Springer New York, p. 92, ISBN 9781441994196.
- ^ Esipov, V. F.; et al. (October 1991), "UBVR Photometry and Rotation of Late Type Galaxies - NGC959 NGC1156 NGC1160 NGC6643 and NGC7292", Soviet Astronomy, 35 (5): 452, Bibcode: 1991SvA....35..452E.
- "Results for object NGC 0959 (NGC 959)". NASA/IPAC Extragalactic Database (NED). California Institute of Technology. Retrieved 2022-01-19.
| NGC 959 | |
|---|---|
|
| |
| Observation data (J2000 epoch) | |
| Constellation | Triangulum |
| Right ascension | 02h 32m 23.923s [1] |
| Declination | +35° 29′ 40.46″ [1] |
| Heliocentric radial velocity | 596 km/s [2] |
| Distance | 36 Mly (11.0 Mpc) [2] [3] |
| Group or cluster | NGC 1023 Group [4] |
| Apparent magnitude (V) | 12.38±0.14 [3] |
| Apparent magnitude (B) | 12.95±0.14 [3] |
| Characteristics | |
| Type | Sdm: [3] or SBcd [5] |
| Mass | 6.3×108 [6] (stellar) M☉ |
| Size | 21.8 kly (6.69 kpc) [7] |
| Apparent size (V) | 2′.3 × 1′.4 [3] (D25) |
| Other designations | |
| IRAS 02293+3516, NGC 959, UGC 2002, LEDA 9665, MCG +06-06-051, PGC 9665 [8] [9] | |
NGC 959 is a spiral galaxy in the northern constellation of Triangulum. [10] It was discovered on November 9, 1876, by French astronomer Édouard Stephan. [9] This galaxy is located at a distance of 36 million light years and is receding with a heliocentric radial velocity of 596 km/s. [2] It is a member of the NGC 1023 Group of galaxies. [4]
The morphological class of this galaxy is Sdm:, [3] indicating it is a spiral (S) with disorganized, irregular arms and no central bulge (dm). The ':' suffix indicates some uncertainty about the classification. It has a visual magnitude of 12.4. [3] The galactic plane is inclined at an angle of 50° to the line of sight from the Earth, [11] giving it an elliptical profile with the major axis aligned along a position angle of 65°. The size of the D25 ellipse (where the brightness of the galaxy drops to magnitude 25) is 2.3 × 1.4 arcminutes. [3]
When images of NGC 959 are corrected for the effects of extinction from dust, a central bar feature can be discerned. The galaxy then shows a non-negligible bulge or central condensation, and may instead have a morphological type of SBcd. [5] It displays a cuspy central density profile and bulge-like monotonic decrease in ellipticity toward the core. [6]
- ^ a b Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv: 1804.09365. Bibcode: 2018A&A...616A...1G. doi: 10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ a b c Tully, R. Brent; et al. (August 2016), "Cosmicflows-3", The Astronomical Journal, 152 (2): 21, arXiv: 1605.01765, Bibcode: 2016AJ....152...50T, doi: 10.3847/0004-6256/152/2/50, S2CID 250737862, 50.
- ^ a b c d e f g h Gil de Paz, Armando; et al. (December 2007), "The GALEX Ultraviolet Atlas of Nearby Galaxies", The Astrophysical Journal Supplement Series, 173 (2): 185–255, arXiv: astro-ph/0606440, Bibcode: 2007ApJS..173..185G, doi: 10.1086/516636, S2CID 119085482.
- ^ a b Trentham, Neil; Tully, R. Brent (September 2009), "Dwarf galaxies in the NGC 1023 Group", Monthly Notices of the Royal Astronomical Society, 398 (2): 722–734, arXiv: 0906.2540, Bibcode: 2009MNRAS.398..722T, doi: 10.1111/j.1365-2966.2009.15189.x, S2CID 18442520.
- ^ a b Tamura, K.; et al. (June 2010), "Lifting the Veil of Dust from NGC 0959: The Importance of a Pixel-based Two-dimensional Extinction Correction", The Astronomical Journal, 139 (6): 2557–2565, arXiv: 1004.3575, Bibcode: 2010AJ....139.2557T, doi: 10.1088/0004-6256/139/6/2557, S2CID 119274723.
- ^ a b Relatores, Nicole C.; et al. (December 2019), "The Dark Matter Distributions in Low-mass Disk Galaxies. II. The Inner Density Profiles", The Astrophysical Journal, 887 (1): 23, arXiv: 1911.05836, Bibcode: 2019ApJ...887...94R, doi: 10.3847/1538-4357/ab5305, S2CID 208006358, 94.
- ^ Truong, Phuongmai N.; et al. (July 2017), "High-resolution Velocity Fields of Low-mass Disk Galaxies. I. CO Observations", The Astrophysical Journal, 843 (1): 15, Bibcode: 2017ApJ...843...37T, doi: 10.3847/1538-4357/aa76eb, S2CID 23645373, 37.
-
^
"NGC 959".
SIMBAD.
Centre de données astronomiques de Strasbourg. Retrieved 2022-01-18.
{{ cite web}}: CS1 maint: postscript ( link) - ^ a b Seligman, Courtney, "NGC Objects: NGC 950 - 999", Celestial Atlas, retrieved 2022-01-18.
- ^ Aranda, Ted (2011), 3,000 Deep-Sky Objects, An Annotated Catalogue, Springer New York, p. 92, ISBN 9781441994196.
- ^ Esipov, V. F.; et al. (October 1991), "UBVR Photometry and Rotation of Late Type Galaxies - NGC959 NGC1156 NGC1160 NGC6643 and NGC7292", Soviet Astronomy, 35 (5): 452, Bibcode: 1991SvA....35..452E.
- "Results for object NGC 0959 (NGC 959)". NASA/IPAC Extragalactic Database (NED). California Institute of Technology. Retrieved 2022-01-19.