NGC 1530
| NGC 1530 | |
|---|---|
NGC 1530 is a
angular separation of 19′.[5]
NGC 1530 has a
″. It includes a clumpy, star-forming nuclear ring structure with a radius of 21″.[9] Star formation is particularly high in the nucleus region and at the ends of the bar, but weak in between these locations.[10] This activity appears to be taking place primarily on the trailing side of the bar where gas pressure is highest.[11] Two linear dust lanes are visible along the bar, which outline shock fronts in the flow of gas.[12]
Mass is flowing into the nuclear ring from the bar at the rate of one solar mass per year[13] with infall velocities of up to 100 km/s.[12] The central region has over 25% of the free gaseous hydrogen in the galaxy.[12] There was some suggestion that the galaxy has a second, inner bar, but this instead appears to be an inner spiral structure. This spiral has one arm brighter than the other, appearing lopsided.[14]
References
- ^ S2CID 18913331.
- ISBN 978-1-4757-4365-4.
- ^ .
- ^ S2CID 118494842, 86.
- ^ ISBN 9781107189485.
- ^ "NGC 1530", SIMBAD, Centre de données astronomiques de Strasbourg, retrieved 2023-02-22.
- ISBN 9781139490108.
- Bibcode:1973rncn.book.....S.
- ^ doi:10.1086/176081.
- Bibcode:1998A&A...337..671R.
- Bibcode:2008ASPC..390..328Z.
- ^ Bibcode:1997A&A...319..737R.
- S2CID 8750099.
- S2CID 12717503.
Further reading
- Popov, Velimir; Ivanov, Emil (2020), "NGC 1530 - type SB(rs)b bared spiral galaxy towards the constellation Camelopardalis", Irida Observatory, retrieved 2023-02-22.
- Randriamampandry, T. H.; et al. (October 2018), "Simulating non-axisymmetric flows in disk galaxies", Astronomy & Astrophysics, 618: A106, S2CID 119230723, A106.
- Zurita, A.; Pérez, I. (July 2008), "Where are the stars of the bar of NGC 1530 forming?", Astronomy and Astrophysics, 485 (1): 5–20, S2CID 14734100.
- Zurita, A.; et al. (January 2004), "Ionized gas kinematics and massive star formation in NGC 1530", Astronomy and Astrophysics, 413: 73–89, S2CID 15585061.
- Zurita, A.; et al. (January 2004), Block, D. L.; et al. (eds.), "High resolution velocity fields in the strongly barred galaxy NGC 1530", Penetrating bars through masks of cosmic dust : the Hubble tuning fork strikes a new note, Proceedings of a conference held at Pilanesburg National Park (South Africa), Astrophysics and space science library (ASSL), vol. 319, Dordrecht: Kluwer Academic Publishers, p. 805, ISBN 978-94-015-7085-5.
- Relaño, M.; et al. (February 2002), Henney, W. J.; et al. (eds.), "High-Velocity Gas in the Luminous H II Regions of NGC 1530", Ionized Gaseous Nebulae, a Conference to Celebrate the 60th Birthdays of Silvia Torres-Peimbert and Manuel Peimbert, Mexico City, November 21-24, 2000, Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias), vol. 12, p. 252, Bibcode:2002RMxAC..12..252R.
- Reynaud, D. (March 2001), "12CO, 13CO and HCN in the Barred Galaxy NGC 1530", Astrophysics and Space Science, 276 (2/4): 619–624, S2CID 117011553.
- Greve, A.; et al. (August 1999), "Stars, H II regions, and shocked gas in the bar of NGC 1530", Astronomy and Astrophysics, 348: 394–404, Bibcode:1999A&A...348..394G.
- Reynaud, D.; Downes, D. (July 1999), "(13) CO(1-0) and (12) CO(2-1) in the center of the barred galaxy NGC 1530", Astronomy and Astrophysics, 347: 37–46, Bibcode:1999A&A...347...37R.
- Regan, Michael W.; et al. (December 1996), "The Morphology of the Stars, Atomic Gas, and Ionized Gas in the Barred Spiral Galaxy NGC 1530", Astronomical Journal, 112: 2549, doi:10.1086/118201.
- Downes, D.; et al. (April 1996), "CO in the Barred Galaxy NGC 1530", Astrophysical Journal, 461: 186, doi:10.1086/177046.