| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Auriga[1] |
| Right ascension | 05h 24m 30.46433s[2] |
| Declination | +42° 44′ 50.4606″[2] |
| Apparent magnitude (V) | 16.1 to 18.5[3] |
| Characteristics | |
| Evolutionary stage | white dwarf + red dwarf[4] |
| Apparent magnitude (G) | 17.115±0.015[5] |
| Apparent magnitude (J) | 16.289±0.096[5] |
| Apparent magnitude (H) | 15.733±0.129[5] |
| Variable type | AM Her/DQ Her[3] |
| Astrometry | |
| Proper motion (μ) | RA: +4.821 mas/yr[2] Dec.: −14.288 mas/yr[2] |
| Parallax (π) | 1.6883±0.0774 mas[2] |
| Distance | 1,930 ± 90 ly (590 ± 30 pc) |
| Orbit | |
| Period (P) | 157.187±0.018 min[6] |
| Details | |
| White dwarf | |
| Mass | 0.74+0.04 −0.05[7] M☉ |
| Radius | 7400+400 −300[7] km |
| Rotation | 136.235±0.025 min[6] |
| Other designations | |
| Paloma, TIC 369210348, 2MASS J05243042+4244506, 1RXS J052430.2+424449,[5] RX J0524+42[8] | |
| Database references | |
| SIMBAD | data |
Paloma is a binary star in the constellation Auriga, at a distance of about 1,930 light-years (590 parsecs). It is a magnetic cataclysmic variable, consisting of a white dwarf accreting material from a companion star. The two stars complete an orbit around each other in just 157 minutes (2.62 hours); the white dwarf has a rotation period of 136 minutes (2.27 hours).[9]
Paloma is a rare intermediate object between polars (AM Herculis stars), which have strong enough magnetic fields to synchronize the spin period of the white dwarf with the orbital period, and intermediate polars (DQ Herculis stars), which have a spin period much shorter than the orbital period. Paloma's spin-orbit ratio places it between these two categories, and it may represent a transitional object – an intermediate polar in the process of synchronizing and becoming a true polar.[8]
The discovery of Paloma (then called RX J0524+42) was first announced at a conference in 2002.[10] The first research paper on the system was published in 2007, which gave it the name Paloma (Spanish for dove or pigeon)[1] in reference to the bird-like shape of the nearby supernova remnant VRO 42.05.01,[8] which is unrelated to Paloma and only appears near it by chance.[9] The name was officially approved by the IAU Working Group on Star Names on 19 April 2026.[1]
References
- "IAU Catalog of Star Names". Retrieved 20 April 2026.
- Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
- "1RXS J052430.2+424449". International Variable Star Index. AAVSO. Retrieved 2026-06-10.
- Joshi, Arti; Pandey, J. C.; et al. (October 2016). "PALOMA: A Magnetic CV between Polars and Intermediate Polars". The Astrophysical Journal. 830 (2): 56. arXiv:1610.00557. Bibcode:2016ApJ...830...56J. doi:10.3847/0004-637X/830/2/56. ISSN 0004-637X.
- "1RXS J052430.2+424449". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 28 May 2026.
- Hernández-Díaz, S.; Stelzer, B.; et al. (November 2025). "A systematic search for orbital periods of polars with TESS: Methods, detection limits, and results". Astronomy & Astrophysics. 703: A166. arXiv:2510.09165. Bibcode:2025A&A...703A.166H. doi:10.1051/0004-6361/202554948. ISSN 0004-6361.
- Dutta, Anirban; Rana, Vikram (December 2022). "Study of Complex Absorption and Reflection in a Unique Intermediate Polar Paloma". The Astrophysical Journal. 940 (2): 100. arXiv:2206.08635. Bibcode:2022ApJ...940..100D. doi:10.3847/1538-4357/ac9587. ISSN 0004-637X.
- Schwarz, R.; Schwope, A. D.; et al. (October 2007). "Paloma (RX J0524+42): the missing link in magnetic CV evolution?". Astronomy & Astrophysics. 473 (2): 511–521. Bibcode:2007A&A...473..511S. doi:10.1051/0004-6361:20077684. ISSN 0004-6361.
- Littlefield, Colin; Hoard, D. W.; et al. (February 2023). "Kepler K2 and TESS Observations of Two Magnetic Cataclysmic Variables: The New Asynchronous Polar SDSS J084617.11+245344.1 and Paloma". The Astronomical Journal. 165 (2): 43. arXiv:2205.02863. Bibcode:2023AJ....165...43L. doi:10.3847/1538-3881/aca1a5. ISSN 0004-6256.
- Warner, Brian (March 2003). "Magnetic Cataclysmic Variables". Publications of the Astronomical Society of the Pacific. 115 (805): 410–411. Bibcode:2003PASP..115..410W. doi:10.1086/368288. ISSN 0004-6280.