Liller 1
| Liller 1 | |
|---|---|
 Liller 1 image from HST | |
| Observation data (J2000 epoch) | |
| Constellation | Scorpius |
| Right ascension | 17h 33m 24.5s[1] |
| Declination | −33° 23′ 20″[1] |
| Distance | 26.4 ± 3.3 kly (8.1 ± 1.0 kpc[2]) |
| Apparent dimensions (V) | 22″ (half-mass diameter) |
| Physical characteristics | |
| Mass | ~2.3×106[2] M☉ |
| Metallicity | = −0.36 dex |
| Other designations | C1730-333, MXB1730-333, J173324.56-332319.8 |
![{\displaystyle {\begin{smallmatrix}\left[{\ce {Fe}}/{\ce {H}}\right]\end{smallmatrix}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/4c0821bd80891e071c08e7c7ee8e022baedf522c)
Liller 1[3] is a globular cluster in the constellation Scorpius, discovered by the American astronomer William Liller in 1977.[3] It is close to the centre of the Milky Way in its galactic bulge, only 2,600 light-years (800 pc) from the centre.[2] Liller 1 is just under 30,000 light years from Earth.[2]
Properties
[edit]Liller 1 is located within the galactic bulge,[2] and is heavily obscured by dust, being close to the galactic plane. Thus, studies of this object have mostly been conducted in wavelengths other than the optical range. The absorbing clouds of dust are not uniform, and the extinction coefficient RV is 2.5, less than the typically assumed value of 3.1.[4]
Liller 1 has a mass of around 2.3 million solar masses; this makes it one of the more massive globular clusters, along with others such as ω Centauri and Terzan 5. After Terzan 5, it has the highest rate of stellar collisions of any Milky Way globular cluster.[2] It also has the highest level of emission of gamma rays of any globular cluster. This may be due to a large number of stellar collisions and pulsars,[5] but it may also be an unrelated background gamma ray source.[2]
Liller 1 and Terzan 5 are remarkably similar. Although globular clusters are typically metal-poor, both have a relatively high metallicity; the abundance of metals for Liller 1 is estimated to be half that of the Sun.[2] In 2021, Liller 1 was found to have two different stellar populations, like Terzan 5.[4] One is about 12 billion years, but the other is relatively young, at 1 to 3 billion years. This suggests that it may not be a true globular cluster, but a class of star cluster that coalesced to form galactic bulges.[6] These star clusters are known as "bulge fossil fragments".[7]
The globular cluster contains the rapid burster called MXB 1730-335.[2]
References
[edit]- ^ a b "C 1730-333". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2015-06-18.
- ^ a b c d e f g h i Saracino, S. (2015). "GEMINI/GeMS observations unveil the structure of the heavily obscured globular cluster Liller 1". The Astrophysical Journal. 806 (2): 152. arXiv:1505.00568. Bibcode:2015ApJ...806..152S. doi:10.1088/0004-637X/806/2/152. S2CID 119034435.
- ^ a b Liller, W (1 April 1977). "Searches for the optical counterparts of the X-ray burst sources MXB 1728-34 and MXB 1730-33". Astrophysical Journal Letters. 213: L21-L23. Bibcode:1977ApJ...213L..21L. doi:10.1086/182401.
- ^ a b Pallanca, Cristina; Ferraro, Francesco R.; Lanzoni, Barbara; Crociati, Chiara; Saracino, Sara; Dalessandro, Emanuele; Origlia, Livia; Rich, Michael R.; Valenti, Elena; Geisler, Douglas; Mauro, Francesco; Villanova, Sandro; Moni Bidin, Christian; Beccari, Giacomo (2021). "High-resolution Extinction Map in the Direction of the Strongly Obscured Bulge Fossil Fragment Liller 1". The Astrophysical Journal. 917 (2): 12. arXiv:2106.02448. Bibcode:2021ApJ...917...92P. doi:10.3847/1538-4357/ac0889. S2CID 235352534. 92.
- ^ Michaud, Peter. "Astronomers image rare stellar cluster Liller 1". PhysOrg. Retrieved 18 June 2015.
- ^ Ferraro, F. R.; Pallanca, C.; Lanzoni, B.; Crociati, C.; Dalessandro, E.; Origlia, L.; Rich, R. M.; Saracino, S.; Mucciarelli, A.; Valenti, E.; Geisler, D.; Mauro, F.; Villanova, S.; Moni Bidin, C.; Beccari, G. (2021). "A new class of fossil fragments from the hierarchical assembly of the Galactic bulge". Nature Astronomy. 5 (3): 311–318. arXiv:2011.09966. Bibcode:2021NatAs...5..311F. doi:10.1038/s41550-020-01267-y. S2CID 227054148.
- ^ Crociati, Chiara; Valenti, Elena; Ferraro, Francesco R.; Pallanca, Cristina; Lanzoni, Barbara; Cadelano, Mario; Fanelli, Cristiano; Origlia, Livia; Leanza, Silvia; Dalessandro, Emanuele; Mucciarelli, Alessio; Rich, R. Michael (2023). "First Evidence of Multi-iron Subpopulations in the Bulge Fossil Fragment Candidate Liller 1". The Astrophysical Journal. 951 (1): 17. arXiv:2305.04595. Bibcode:2023ApJ...951...17C. doi:10.3847/1538-4357/acd382.