ZTF J0328-1219
.png){kind=spacer} ZTF J0328−1219 phase-fitted light curve with McDonald Observatory (solid circles) and SAAO (open circles) Credit: Vanderbosch et al. 2021[1] | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Eridanus |
| Right ascension | 03h 28m 33.52s |
| Declination | −12° 19′ 45.26″ |
| Characteristics | |
| Evolutionary stage | white dwarf |
| Spectral type | DZ[2] |
| Variable type | transiting debris[1] |
| Astrometry | |
| Radial velocity (Rv) | 58.8 ±0.8[1] km/s |
| Proper motion (μ) | RA: 110.739 ±0.055 mas/yr[1] Dec.: −14.39 ±0.046 mas/yr[1] |
| Parallax (π) | 23.038 ± 0.056 mas[1] |
| Distance | 141.6 ± 0.3 ly (43.4 ± 0.1 pc) |
| Details[1] | |
| Mass | 0.731 ±0.023 M☉ |
| Radius | 0.0107 ±0.0002 R☉ |
| Radius | 7444 ±139 km |
| Surface gravity (log g) | 8.245 ±0.035 cgs |
| Temperature | 7630 ±140 K |
| Metallicity | [Ca/He] =−9.55 ±0.12 |
| Age | cooling age: 1.84 ±0.17 Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
ZTF J032833.52−121945.27 (also called ZTF J0328-1219) is a white dwarf with two transiting debris clouds around it.[1]
ZTF J0328-1219 was first discovered as a white dwarf with Gaia and the virtual observatory in 2018. At the time it was known by its Gaia identification number.[3] In 2021 it was discovered that this white dwarf has transiting debris around it. This was discovered with the Zwicky Transient Facility (ZTF) and follow-up photometry with the McDonald Observatory. It was also shown with spectroscopy from the Lowell Discovery Telescope (LDT) that the white dwarf has deep calcium absorption lines.[2]
A more detailed study was published in 2021. Photometry was obtained with the TESS, ZTF, McDonald Observatory, SAAO, HAO, and JBO. Spectroscopy was obtained with SOAR, Magellan and the archived LDT spectrum. From the photometry the researchers find two significant periods at 9.937 and 11.2 hours (A-period and B-period). The dips change on nightly, weekly and monthly timescales. The researchers detected calcium, sodium, both with circumstellar origin. The sodium line is blueshifted by 21.4 ±1.0 km/s compared to the atmospheric lines. The researchers also identified atmospheric Hydrogen-alpha absorption. Due to the low amount of hydrogen, the researchers assume a helium dominated atmosphere. The variability of ZTF J0328-1219 is similar to WD 1145+017, but with notable differences. ZTF J0328-1219 is continuously variable, suggesting dust clouds orbit the white dwarf. These dust clouds either orbit the white dwarf on their own, or they are emitted by one or more bodies.[1]
The two dust clouds would have semi-major axes of 2.11 and 2.28 R☉. An orbiting exocomet is less likely because it would completely evaporate at this orbit within a few years. An orbiting exoasteroid on the other hand would not evaporate at this orbit. At the 9.93 hour orbit a body would be heated to a temperature of 700 Kelvin (K), but most minerals of asteroids evaporate at 1500-2500 K. The researchers propose several solutions for this problem:[1]
- Fine material ejected during collisions from bodies orbiting in a dust ring
- Volatiles below the surface are heated and eject overlaying material (similar to some active asteroids in the solar system)
- An exocomet with deep pits that preserve volatiles for later times
- An exocomet orbiting within a dusty disk, shielding the comet from radiation, lowering the temperature
- An exoasteroid with an eccentric orbit that will peel off material during periastron passage
- A cascade of collisions beginning with the collision of two bodies
Observations of ZTF J0328-1219 showed a long-term fading event. The white dwarf faded by around 0.3 mag between 2012 and 2014. This is interpreted as increased transit activity during this time. This discovery is based on observations with the Thai National Telescope.[4]
See also
[edit]- List of stars that have unusual dimming periods
- List of exoplanets and planetary debris around white dwarfs
References
[edit]- ^ a b c d e f g h i Vanderbosch, Zachary P.; Rappaport, Saul; Guidry, Joseph A.; Gary, Bruce L.; Blouin, Simon; Kaye, Thomas G.; Weinberger, Alycia J.; Melis, Carl; Klein, Beth L.; Zuckerman, B.; Vanderburg, Andrew; Hermes, J. J.; Hegedus, Ryan J.; Burleigh, Matthew. R.; Sefako, Ramotholo (2021-08-01). "Recurring Planetary Debris Transits and Circumstellar Gas around White Dwarf ZTF J0328-1219". The Astrophysical Journal. 917 (1): 41. arXiv:2106.02659. Bibcode:2021ApJ...917...41V. doi:10.3847/1538-4357/ac0822. ISSN 0004-637X. S2CID 235358242.
- ^ a b Guidry, Joseph A.; Vanderbosch, Zachary P.; Hermes, J. J.; Barlow, Brad N.; Lopez, Isaac D.; Boudreaux, Thomas M.; Corcoran, Kyle A.; Bell, Keaton J.; Montgomery, M. H.; Heintz, Tyler M.; Castanheira, Barbara G.; Reding, Joshua S.; Dunlap, Bart H.; Winget, D. E.; Winget, Karen I. (2021-05-01). "I Spy Transits and Pulsations: Empirical Variability in White Dwarfs Using Gaia and the Zwicky Transient Facility". The Astrophysical Journal. 912 (2): 125. arXiv:2012.00035. Bibcode:2021ApJ...912..125G. doi:10.3847/1538-4357/abee68. ISSN 0004-637X. S2CID 227238802.
- ^ Jiménez-Esteban, F. M.; Torres, S.; Rebassa-Mansergas, A.; Skorobogatov, G.; Solano, E.; Cantero, C.; Rodrigo, C. (2018-11-01). "A white dwarf catalogue from Gaia-DR2 and the Virtual Observatory". Monthly Notices of the Royal Astronomical Society. 480 (4): 4505–4518. arXiv:1807.02559. Bibcode:2018MNRAS.480.4505J. doi:10.1093/mnras/sty2120. ISSN 0035-8711.
- ^ Aungwerojwit, Amornrat; Gänsicke, Boris T.; Dhillon, Vikram S.; Drake, Andrew; Inight, Keith; Kaye, Thomas G.; Marsh, T. R.; Mullen, Ed; Pelisoli, Ingrid; Swan, Andrew (2024-05-01). "Long-term variability in debris transiting white dwarfs". Monthly Notices of the Royal Astronomical Society. 530 (1): 117–128. arXiv:2404.04422. Bibcode:2024MNRAS.530..117A. doi:10.1093/mnras/stae750. ISSN 0035-8711.
External links
[edit]- J0328-1219 observations with the Hereford Arizona Observatory (HAO) by amateur Bruce L. Gary, page 1 (page 2 and season 3, 4 are chain-linked within page 1)
- Press release by the Boston University white dwarf group