Discovery of Two New Eruptions of the Ultrashort Recurrence Time Nova M31N 2017-01e*

Abstract We report the recent discovery of two new eruptions of the recurrent nova M31N 2017-01e in the Andromeda galaxy. The latest eruption, M31N 2024-08c, reached R = 17.8 on 2024 August 06.85 UT, ∼2 months earlier than predicted. In addition to this recent eruption, a search of archival Palomar Transient Factory data has revealed a previously unreported eruption on 2014 June 18.46 UT that reached a peak brightness of R ∼ 17.9 approximately a day later. The addition of these two eruption timings has allowed us to update the mean recurrence time of the nova. We find 〈 T rec 〉 = 924.0 ± 7.0 days (2.53 ± 0.02 yr), which is slightly shorter than our previous determination. Thus, M31N 2017-01e remains the nova with the second shortest recurrence time known, with only M31N 2008-12a being shorter. We also present a low-resolution spectrum of the likely quiescent counterpart of the nova, a ∼20.5 mag evolved B star displaying an ∼14.3 days photometric modulation.

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Publication Details

Journal
Research Notes of the AAS
Published
2024-10-10
DOI
https://doi.org/10.3847/2515-5172/ad84d5
Citations
3
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
1.98
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article

Discovery of Two New Eruptions of the Ultrashort Recurrence Time Nova M31N 2017-01e*

H. Kučáková, Howard E. Bond, M. Zhang, Wei-Hao Wang et al.
3 citations
Research Notes of the AAS
Astrophysics and Cosmic Phenomena
1.98
article

Discovery of Two New Eruptions of the Ultrashort Recurrence Time Nova M31N 2017-01e*

H. Kučáková, Howard E. Bond, M. Zhang, Wei-Hao Wang, A. W. Shafter, K. Hornoch, Kenta Taguchi, R. E. Williams, Gregory R. Zeimann, Jingyuan Zhao, Weiye 炜晔 Wang 王, Yuqing 育庆 Ren 任, Lanhe 岚贺 Ding 丁, Xiaochang 小畅 Yan 严, Jiashuo 家硕 Zhang 张, Jia 嘉 You 游, Binyu 彬羽 Wang 王, Runwei 润玮 Xu 许
article en
3 citations

Abstract

Abstract We report the recent discovery of two new eruptions of the recurrent nova M31N 2017-01e in the Andromeda galaxy. The latest eruption, M31N 2024-08c, reached R = 17.8 on 2024 August 06.85 UT, ∼2 months earlier than predicted. In addition to this recent eruption, a search of archival Palomar Transient Factory data has revealed a previously unreported eruption on 2014 June 18.46 UT that reached a peak brightness of R ∼ 17.9 approximately a day later. The addition of these two eruption timings has allowed us to update the mean recurrence time of the nova. We find 〈 T rec 〉 = 924.0 ± 7.0 days (2.53 ± 0.02 yr), which is slightly shorter than our previous determination. Thus, M31N 2017-01e remains the nova with the second shortest recurrence time known, with only M31N 2008-12a being shorter. We also present a low-resolution spectrum of the likely quiescent counterpart of the nova, a ∼20.5 mag evolved B star displaying an ∼14.3 days photometric modulation.

Research Notes of the AASVol. 8(10)
Space Telescope Science Institute (US), Pennsylvania State University (US), Okayama University (JP), University of California, Santa Cruz (US), Charles University (CZ), Kyoto University (JP), San Diego State University (US), Czech Academy of Sciences, Astronomical Institute (CZ), The University of Texas at Austin (US)
Openalex Percentile: Top 9%
Astrophysics and Cosmic Phenomena
1.98
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