The Curious Case of PHL 293B : a long-lived transient in a Metal-poor Blue Compact Dwarf Galaxy
Main Author: | |
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Publication Date: | 2020 |
Other Authors: | , |
Format: | Article |
Language: | eng |
Source: | Repositório Institucional da UFRGS |
Download full: | http://hdl.handle.net/10183/212323 |
Summary: | We report on small-amplitude optical variability and recent dissipation of the unusually persistent broad emission lines in the blue compact dwarf galaxy PHL 293B. The galaxy's unusual spectral features (P Cygni-like profiles with ~800 km s−1 blueshifted absorption lines) have resulted in conflicting interpretations of the nature of this source in the literature. However, analysis of new Gemini spectroscopy reveals the broad emission has begun to fade after being persistent for over a decade prior. Precise difference imaging light curves constructed with the Sloan Digital Sky Survey and the Dark Energy Survey reveal small-amplitude optical variability of ~0.1 mag in the g band offset by 100 ± 21 pc from the brightest pixel of the host. The light curve is well-described by an active galactic nuclei (AGN)-like damped random walk process. However, we conclude that the origin of the optical variability and spectral features of PHL 293B is due to a long-lived stellar transient, likely a Type IIn supernova or nonterminal outburst, mimicking long-term AGN-like variability. This work highlights the challenges of discriminating between scenarios in such extreme environments, relevant to searches for AGNs in dwarf galaxies. This is the second long-lived transient discovered in a blue compact dwarf, after SDSS1133. Our result implies such long-lived stellar transients may be more common in metal-deficient galaxies. Systematic searches for low-level variability in dwarf galaxies will be possible with the upcoming Legacy Survey of Space and Time at the Vera C. Rubin Observatory. |
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Burke, Colin J.Santiago, Basilio XavierDES Collaboration2020-07-23T03:40:12Z20200004-637Xhttp://hdl.handle.net/10183/212323001114799We report on small-amplitude optical variability and recent dissipation of the unusually persistent broad emission lines in the blue compact dwarf galaxy PHL 293B. The galaxy's unusual spectral features (P Cygni-like profiles with ~800 km s−1 blueshifted absorption lines) have resulted in conflicting interpretations of the nature of this source in the literature. However, analysis of new Gemini spectroscopy reveals the broad emission has begun to fade after being persistent for over a decade prior. Precise difference imaging light curves constructed with the Sloan Digital Sky Survey and the Dark Energy Survey reveal small-amplitude optical variability of ~0.1 mag in the g band offset by 100 ± 21 pc from the brightest pixel of the host. The light curve is well-described by an active galactic nuclei (AGN)-like damped random walk process. However, we conclude that the origin of the optical variability and spectral features of PHL 293B is due to a long-lived stellar transient, likely a Type IIn supernova or nonterminal outburst, mimicking long-term AGN-like variability. This work highlights the challenges of discriminating between scenarios in such extreme environments, relevant to searches for AGNs in dwarf galaxies. This is the second long-lived transient discovered in a blue compact dwarf, after SDSS1133. Our result implies such long-lived stellar transients may be more common in metal-deficient galaxies. Systematic searches for low-level variability in dwarf galaxies will be possible with the upcoming Legacy Survey of Space and Time at the Vera C. Rubin Observatory.application/pdfengThe astrophysical journal. Bristol. Vol. 894, no. 1 (May 2020), L5, 11 p.SupernovaEstrelas variaveisGaláxias anãsType II supernovaeTransient detectionLuminous blue variable starsBlue compact dwarf galaxiesDwarf galaxiesGalaxiesThe Curious Case of PHL 293B : a long-lived transient in a Metal-poor Blue Compact Dwarf GalaxyEstrangeiroinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UFRGSinstname:Universidade Federal do Rio Grande do Sul (UFRGS)instacron:UFRGSTEXT001114799.pdf.txt001114799.pdf.txtExtracted Texttext/plain54270http://www.lume.ufrgs.br/bitstream/10183/212323/2/001114799.pdf.txt114d8a740760b1328b3db0faf72877fcMD52ORIGINAL001114799.pdfTexto completo (inglês)application/pdf972572http://www.lume.ufrgs.br/bitstream/10183/212323/1/001114799.pdfa717aa1236a12625b444661e99ed0578MD5110183/2123232023-07-02 03:40:50.047447oai:www.lume.ufrgs.br:10183/212323Repositório InstitucionalPUBhttps://lume.ufrgs.br/oai/requestlume@ufrgs.bropendoar:2023-07-02T06:40:50Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false |
dc.title.pt_BR.fl_str_mv |
The Curious Case of PHL 293B : a long-lived transient in a Metal-poor Blue Compact Dwarf Galaxy |
title |
The Curious Case of PHL 293B : a long-lived transient in a Metal-poor Blue Compact Dwarf Galaxy |
spellingShingle |
The Curious Case of PHL 293B : a long-lived transient in a Metal-poor Blue Compact Dwarf Galaxy Burke, Colin J. Supernova Estrelas variaveis Galáxias anãs Type II supernovae Transient detection Luminous blue variable stars Blue compact dwarf galaxies Dwarf galaxies Galaxies |
title_short |
The Curious Case of PHL 293B : a long-lived transient in a Metal-poor Blue Compact Dwarf Galaxy |
title_full |
The Curious Case of PHL 293B : a long-lived transient in a Metal-poor Blue Compact Dwarf Galaxy |
title_fullStr |
The Curious Case of PHL 293B : a long-lived transient in a Metal-poor Blue Compact Dwarf Galaxy |
title_full_unstemmed |
The Curious Case of PHL 293B : a long-lived transient in a Metal-poor Blue Compact Dwarf Galaxy |
title_sort |
The Curious Case of PHL 293B : a long-lived transient in a Metal-poor Blue Compact Dwarf Galaxy |
author |
Burke, Colin J. |
author_facet |
Burke, Colin J. Santiago, Basilio Xavier DES Collaboration |
author_role |
author |
author2 |
Santiago, Basilio Xavier DES Collaboration |
author2_role |
author author |
dc.contributor.author.fl_str_mv |
Burke, Colin J. Santiago, Basilio Xavier DES Collaboration |
dc.subject.por.fl_str_mv |
Supernova Estrelas variaveis Galáxias anãs |
topic |
Supernova Estrelas variaveis Galáxias anãs Type II supernovae Transient detection Luminous blue variable stars Blue compact dwarf galaxies Dwarf galaxies Galaxies |
dc.subject.eng.fl_str_mv |
Type II supernovae Transient detection Luminous blue variable stars Blue compact dwarf galaxies Dwarf galaxies Galaxies |
description |
We report on small-amplitude optical variability and recent dissipation of the unusually persistent broad emission lines in the blue compact dwarf galaxy PHL 293B. The galaxy's unusual spectral features (P Cygni-like profiles with ~800 km s−1 blueshifted absorption lines) have resulted in conflicting interpretations of the nature of this source in the literature. However, analysis of new Gemini spectroscopy reveals the broad emission has begun to fade after being persistent for over a decade prior. Precise difference imaging light curves constructed with the Sloan Digital Sky Survey and the Dark Energy Survey reveal small-amplitude optical variability of ~0.1 mag in the g band offset by 100 ± 21 pc from the brightest pixel of the host. The light curve is well-described by an active galactic nuclei (AGN)-like damped random walk process. However, we conclude that the origin of the optical variability and spectral features of PHL 293B is due to a long-lived stellar transient, likely a Type IIn supernova or nonterminal outburst, mimicking long-term AGN-like variability. This work highlights the challenges of discriminating between scenarios in such extreme environments, relevant to searches for AGNs in dwarf galaxies. This is the second long-lived transient discovered in a blue compact dwarf, after SDSS1133. Our result implies such long-lived stellar transients may be more common in metal-deficient galaxies. Systematic searches for low-level variability in dwarf galaxies will be possible with the upcoming Legacy Survey of Space and Time at the Vera C. Rubin Observatory. |
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2020 |
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2020-07-23T03:40:12Z |
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2020 |
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001114799 |
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The astrophysical journal. Bristol. Vol. 894, no. 1 (May 2020), L5, 11 p. |
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