| NGC 7507 | |
|---|---|
 NGC 7507 (2MASS) | |
| Observation data (J2000 epoch) | |
| Constellation | Sculptor |
| Right ascension | 23 12 07.595 |
| Declination | −28° 32′ 22.70″ |
| Redshift | 0.005260±0.000100 |
| Heliocentric radial velocity | 1,590±21 km/s |
| Distance | 80.07 ± 0.46 Mly (24.55 ± 0.14 Mpc) |
| Apparent magnitude (V) | 10.6 |
| Apparent magnitude (B) | 11.60 |
| Characteristics | |
| Type | E0 |
| Mass | 2×10 M☉ |
| Size | 91 kly |
| Apparent size (V) | 1.987′ × 1.907′ (NIR) |
| Other designations | |
| NGC 7507, LEDA 70676, MCG -05-54-022; ESO 469-19, AM 2309-284 | |
NGC 7507 is an elliptical galaxy located in the constellation Sculptor. It was discovered by the German-British astronomer William Herschel on October 30, 1783. The galaxy lies at an estimated distance of 80.1 million light-years (24.55 Mpc) from the Milky Way, and has an angular size of 2.0′ × 1.9′ in the near infrared. It is receding with a heliocentric radial velocity of 1,590 km/s.
The morphological classification of NGC 7507 is E0, indicating an elliptical galaxy with an almost perfectly circular profile. This massive galaxy is fairly isolated, although it forms a pair with the barred spiral galaxy NGC 7513. The latter lies at a projected angular separation of 18′. Apart from a central dust lane, NGC 7507 displays neither shells nor tidal features. The stellar halo has two components, with the outer and inner halos counter-rotating.
It is unusual galaxy in that it displays a negligible dark matter profile, showing a constant mass to light ratio. This apparent lack of a dark matter component is difficult to explain in an LCDM cosmology. The globular cluster population around NGC 7507 is very small, being only a tenth the size of other comparable ellipticals. It more closely resembles the globular population of a spiral galaxy.
References
- ^ Skrutskie, Michael F.; et al. (February 1, 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. ISSN 0004-6256. S2CID 18913331.
- Paturel, G.; et al. (2002). Comparison LEDA/SIMBAD octobre 2002. Catalogue to be published in 2003. Bibcode:2002LEDA.........0P.
- ^ Ogando, Ricardo L. C.; et al. (June 2008). "Line Strengths of Early-Type Galaxies". The Astronomical Journal. 135 (6): 2424–2445. arXiv:0803.3477. Bibcode:2008AJ....135.2424O. doi:10.1088/0004-6256/135/6/2424.
- ^ Tully, R. Brent; et al. (October 2013). "Cosmicflows-2: The Data". The Astronomical Journal. 146 (4): 25. arXiv:1307.7213. Bibcode:2013AJ....146...86T. doi:10.1088/0004-6256/146/4/86. S2CID 118494842. 86.
- ^ Simpson, Phil (2012). Guidebook to the Constellations: Telescopic Sights, Tales, and Myths. The Patrick Moore Practical Astronomy Series. Springer Science & Business Media. p. 800. ISBN 9781441969415.
- Lauberts, A.; Valentijn, E. A. (1989). The Surface Photometry Catalogue of the ESO-Uppsala Galaxies. Bibcode:1989spce.book.....L.
- "NASA/IPAC Extragalactic Database". Results for NGC 7507. Retrieved 2020-01-17.
- ^ Salinas, R.; et al. (February 2012). "Kinematic properties of the field elliptical NGC 7507". Astronomy & Astrophysics. 538. id. A87. arXiv:1111.1581. Bibcode:2012A&A...538A..87S. doi:10.1051/0004-6361/201116517.
- "NGC 7507". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-01-17.
- Seligman, Courtney. "New General Catalog Objects: NGC 7500 - 7549". cseligman.com. Retrieved 2024-09-30.
- ^ Caso, J. P.; et al. (July 2013). "The paucity of globular clusters around the field elliptical NGC 7507". Astronomy & Astrophysics. 555. id. A56. arXiv:1305.1335. Bibcode:2013A&A...555A..56C. doi:10.1051/0004-6361/201321032.
- ^ Lane, Richard R.; et al. (February 2015). "Dark matter deprivation in the field elliptical galaxy NGC 7507". Astronomy & Astrophysics. 574. id. A93. arXiv:1412.3402. Bibcode:2015A&A...574A..93L. doi:10.1051/0004-6361/201424074.