The Curious Case of ASASSN-20hx: A Slowly-Evolving, UV and X-ray Luminous, Ambiguous Nuclear Transient
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2021
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| author | Hinkle, Jason T. Holoien, Thomas W. -S. Shappee, Benjamin. J. Neustadt, Jack M. M. Auchettl, Katie Vallely, Patrick J. Shahbandeh, Melissa Kluge, Matthias Kochanek, Christopher S. Stanek, K. Z. Huber, Mark E. Post, Richard S. Bersier, David Ashall, Christopher Tucker, Michael A. Williams, Jonathan P. de Jaeger, Thomas Do, Aaron Fausnaugh, Michael Gruen, Daniel Hopp, Ulrich Myles, Justin Obermeier, Christian Payne, Anna V. Thompson, Todd A. |
| author_facet | Hinkle, Jason T. Holoien, Thomas W. -S. Shappee, Benjamin. J. Neustadt, Jack M. M. Auchettl, Katie Vallely, Patrick J. Shahbandeh, Melissa Kluge, Matthias Kochanek, Christopher S. Stanek, K. Z. Huber, Mark E. Post, Richard S. Bersier, David Ashall, Christopher Tucker, Michael A. Williams, Jonathan P. de Jaeger, Thomas Do, Aaron Fausnaugh, Michael Gruen, Daniel Hopp, Ulrich Myles, Justin Obermeier, Christian Payne, Anna V. Thompson, Todd A. |
| contents | We present observations of ASASSN-20hx, a nearby ambiguous nuclear transient (ANT) discovered in NGC 6297 by the All-Sky Automated Survey for Supernovae (ASAS-SN). We observed ASASSN-20hx from $-$30 to 275 days relative to peak UV/optical emission using high-cadence, multi-wavelength spectroscopy and photometry. From Transiting Exoplanet Survey Satellite (TESS) data, we determine that the ANT began to brighten on 2020 June 22.8 with a linear rise in flux for at least the first week. ASASSN-20hx peaked in the UV/optical 30 days later on 2020 July 22.8 (MJD = 59052.8) at a bolometric luminosity of $L = (3.15 \pm 0.04) \times 10^{43}$ erg s$^{-1}$. The subsequent decline is slower than any TDE observed to date and consistent with many other ANTs. Compared to an archival X-ray detection, the X-ray luminosity of ASASSN-20hx increased by an order of magnitude to $L_{x} \sim 1.5 \times 10^{42}$ erg s$^{-1}$ and then slowly declined over time. The X-ray emission is well-fit by a power law with a photon index of $Γ\sim 2.3 - 2.6$. Both the optical and near infrared spectra of ASASSN-20hx lack emission lines, unusual for any known class of nuclear transient. While ASASSN-20hx has some characteristics seen in both tidal disruption events (TDEs) and active galactic nuclei (AGNs), it cannot be definitively classified with current data. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2108_03245 |
| institution | arXiv |
| publishDate | 2021 |
| record_format | arxiv |
| spellingShingle | The Curious Case of ASASSN-20hx: A Slowly-Evolving, UV and X-ray Luminous, Ambiguous Nuclear Transient Hinkle, Jason T. Holoien, Thomas W. -S. Shappee, Benjamin. J. Neustadt, Jack M. M. Auchettl, Katie Vallely, Patrick J. Shahbandeh, Melissa Kluge, Matthias Kochanek, Christopher S. Stanek, K. Z. Huber, Mark E. Post, Richard S. Bersier, David Ashall, Christopher Tucker, Michael A. Williams, Jonathan P. de Jaeger, Thomas Do, Aaron Fausnaugh, Michael Gruen, Daniel Hopp, Ulrich Myles, Justin Obermeier, Christian Payne, Anna V. Thompson, Todd A. High Energy Astrophysical Phenomena We present observations of ASASSN-20hx, a nearby ambiguous nuclear transient (ANT) discovered in NGC 6297 by the All-Sky Automated Survey for Supernovae (ASAS-SN). We observed ASASSN-20hx from $-$30 to 275 days relative to peak UV/optical emission using high-cadence, multi-wavelength spectroscopy and photometry. From Transiting Exoplanet Survey Satellite (TESS) data, we determine that the ANT began to brighten on 2020 June 22.8 with a linear rise in flux for at least the first week. ASASSN-20hx peaked in the UV/optical 30 days later on 2020 July 22.8 (MJD = 59052.8) at a bolometric luminosity of $L = (3.15 \pm 0.04) \times 10^{43}$ erg s$^{-1}$. The subsequent decline is slower than any TDE observed to date and consistent with many other ANTs. Compared to an archival X-ray detection, the X-ray luminosity of ASASSN-20hx increased by an order of magnitude to $L_{x} \sim 1.5 \times 10^{42}$ erg s$^{-1}$ and then slowly declined over time. The X-ray emission is well-fit by a power law with a photon index of $Γ\sim 2.3 - 2.6$. Both the optical and near infrared spectra of ASASSN-20hx lack emission lines, unusual for any known class of nuclear transient. While ASASSN-20hx has some characteristics seen in both tidal disruption events (TDEs) and active galactic nuclei (AGNs), it cannot be definitively classified with current data. |
| title | The Curious Case of ASASSN-20hx: A Slowly-Evolving, UV and X-ray Luminous, Ambiguous Nuclear Transient |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2108.03245 |