The only inflated brown dwarf in an eclipsing white dwarf-brown dwarf binary: WD1032+011B
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arXiv
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2024
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| author | French, Jenni R. Casewell, Sarah L. Amaro, Rachael C. Lothringer, Joshua D. Mayorga, L. C. Littlefair, Stuart P. Lew, Ben W. P. Zhou, Yifan Apai, Daniel Marley, Mark S. Parmentier, Vivien Tan, Xianyu |
| author_facet | French, Jenni R. Casewell, Sarah L. Amaro, Rachael C. Lothringer, Joshua D. Mayorga, L. C. Littlefair, Stuart P. Lew, Ben W. P. Zhou, Yifan Apai, Daniel Marley, Mark S. Parmentier, Vivien Tan, Xianyu |
| contents | Due to their short orbital periods and relatively high flux ratios, irradiated brown dwarfs in binaries with white dwarfs offer better opportunities to study irradiated atmospheres than hot Jupiters, which have lower planet-to-star flux ratios. WD1032+011 is an eclipsing, tidally locked white dwarf-brown dwarf binary with a 9950 K white dwarf orbited by a 69.7 M$_{Jup}$ brown dwarf in a 0.09 day orbit. We present time-resolved Hubble Space Telescope Wide Field Camera 3 spectrophotometric data of WD1032+011. We isolate the phase-dependent spectra of WD1032+011B, finding a 210 K difference in brightness temperature between the dayside and nightside. The spectral type of the brown dwarf is identified as L1 peculiar, with atmospheric retrievals and comparison to field brown dwarfs showing evidence for a cloud-free atmosphere. The retrieved temperature of the dayside is $1748^{+66}_{-67}$ K, with a nightside temperature of $1555^{+76}_{-62}$ K, showing an irradiation-driven temperature contrast coupled with inefficient heat redistribution from the dayside to the nightside. The brown dwarf radius is inflated, likely due to the constant irradiation from the white dwarf, making it the only known inflated brown dwarf in an eclipsing white dwarf-brown dwarf binary. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2409_06874 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | The only inflated brown dwarf in an eclipsing white dwarf-brown dwarf binary: WD1032+011B French, Jenni R. Casewell, Sarah L. Amaro, Rachael C. Lothringer, Joshua D. Mayorga, L. C. Littlefair, Stuart P. Lew, Ben W. P. Zhou, Yifan Apai, Daniel Marley, Mark S. Parmentier, Vivien Tan, Xianyu Solar and Stellar Astrophysics Earth and Planetary Astrophysics Due to their short orbital periods and relatively high flux ratios, irradiated brown dwarfs in binaries with white dwarfs offer better opportunities to study irradiated atmospheres than hot Jupiters, which have lower planet-to-star flux ratios. WD1032+011 is an eclipsing, tidally locked white dwarf-brown dwarf binary with a 9950 K white dwarf orbited by a 69.7 M$_{Jup}$ brown dwarf in a 0.09 day orbit. We present time-resolved Hubble Space Telescope Wide Field Camera 3 spectrophotometric data of WD1032+011. We isolate the phase-dependent spectra of WD1032+011B, finding a 210 K difference in brightness temperature between the dayside and nightside. The spectral type of the brown dwarf is identified as L1 peculiar, with atmospheric retrievals and comparison to field brown dwarfs showing evidence for a cloud-free atmosphere. The retrieved temperature of the dayside is $1748^{+66}_{-67}$ K, with a nightside temperature of $1555^{+76}_{-62}$ K, showing an irradiation-driven temperature contrast coupled with inefficient heat redistribution from the dayside to the nightside. The brown dwarf radius is inflated, likely due to the constant irradiation from the white dwarf, making it the only known inflated brown dwarf in an eclipsing white dwarf-brown dwarf binary. |
| title | The only inflated brown dwarf in an eclipsing white dwarf-brown dwarf binary: WD1032+011B |
| topic | Solar and Stellar Astrophysics Earth and Planetary Astrophysics |
| url | https://arxiv.org/abs/2409.06874 |