IC 4588 is a type E[1] elliptical galaxy located in the constellation Serpens.[2][3] It is located 729 million light-years from the Solar System[4] and has a dimension of 0.30 x 0.3 arcmin meaning its diameter is 64,000 light-years across.[5] IC 4588 was discovered by Stephane Javelle on July 15, 1903.[6]
| IC 4588 | |
|---|---|
 | |
| Observation data (J2000 epoch) | |
| Constellation | Serpens |
| Right ascension | 16h 05m 04.24s |
| Declination | +23° 55′ 01.69″ |
| Redshift | 0.053096 |
| Heliocentric radial velocity | 15,918 km/s |
| Distance | 729 Mly (223.5 Mpc) |
| Apparent magnitude (V) | 15.8 |
| Characteristics | |
| Type | E |
| Size | 64,000 ly |
| Apparent size (V) | 0.30′ × 0.3′ |
| Other designations | |
| 2MASS J16050425+2355015, 2MASX J16050427+2355015, LEDA 57025, PGC 57025, SDSS J160504.24+235501.6 | |
In some galactic catalogues, NGC 6051 and IC 4588 have been listed as the same object.[7] However, O'Sullivan and associates (2011) have them as separate entities, with NGC 6051 being the central dominant galaxy of a cluster.[8]
Supernova
editOne supernova has been discovered in IC 4588 so far: SN 2023ifv.
SN 2023ifv
SN 2023ifv was discovered on May 13, 2023[9] by ATLAS (Asteroid Terrestrial-impact Last Alert System) which was developed by the University of Hawaii.[10] It was reported by multiple astronomers from University of Hawaii, South African Astronomical Observatory, ESO, UAI Obstech, Oxford/QUB, Queen's University Belfast, Oxford and Harvard; via a cyan-ATLAS filter which was taken using ATLAS Haleakala telescope.[11] The supernova reached a magnitude of 18.[12]
On May 19, 2023, C. Fremling, D. Neill, and Y. Sharma on the behalf of the SDEM Team from Caltech and the Zwicky Transient Facility, confirmed SN 2023ifv to be a Type Ia supernova.[13][14] The supernova probably resulted from the destruction of a white dwarf in a binary system.[15][16]
References
edit- ^ "HyperLeda -object description". atlas.obs-hp.fr. Retrieved 2024-05-08.
- ^ Astronomy, Go. "IC 4588 | galaxy in Serpens | IC List | GO ASTRONOMY". Go-Astronomy.com. Retrieved 2024-05-08.
- ^ Ford, Dominic. "IC4588 (Galaxy)". In-The-Sky.org. Retrieved 2024-05-08.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-05-08.
- ^ "Revised IC Data for IC 4588". spider.seds.org. Retrieved 2024-05-08.
- ^ "Index Catalog Objects: IC 4550 - 4599". cseligman.com. Retrieved 2024-05-08.
- ^ "IC 4588". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-06-27.
- ^ O'Sullivan, Ewan; et al. (March 2011). "A deep Chandra observation of the poor cluster AWM 4 - II. The role of the radio jets in enriching the intracluster medium". Monthly Notices of the Royal Astronomical Society. 411 (3): 1833–1842. arXiv:1010.0610. Bibcode:2011MNRAS.411.1833O. doi:10.1111/j.1365-2966.2010.17812.x.
- ^ "Lasair. A UK Alert Stream Broker and Transient Science Platform". metatags.io. Retrieved 2024-05-08.
- ^ "ATLAS - The ATLAS Project". atlas.fallingstar.com. Retrieved 2024-05-08.
- ^ "Discovery certificate for object 2023ifv | Transient Name Server". www.wis-tns.org. Retrieved 2024-05-08.
- ^ "Bright Supernovae - 2023". www.rochesterastronomy.org. Retrieved 2024-05-08.
- ^ "Classification certificate for object 2023ifv | Transient Name Server". www.wis-tns.org. Retrieved 2024-05-08.
- ^ "SN 2023ifv | Transient Name Server". www.wis-tns.org. Retrieved 2024-05-08.
- ^ Liu, Zheng-Wei; Röpke, Friedrich K.; Han, Zhanwen (2023-08-01). "Type Ia Supernova Explosions in Binary Systems: A Review". Research in Astronomy and Astrophysics. 23 (8): 082001. arXiv:2305.13305. Bibcode:2023RAA....23h2001L. doi:10.1088/1674-4527/acd89e. ISSN 1674-4527.
- ^ Maguire, Kate (2016), Alsabti, Athem W.; Murdin, Paul (eds.), "Type Ia Supernovae", Handbook of Supernovae, Cham: Springer International Publishing, pp. 1–24, doi:10.1007/978-3-319-20794-0_36-1, ISBN 978-3-319-20794-0, retrieved 2024-05-08