TY - JOUR
T1 - Godzilla, a monster lurks in the Sunburst galaxy
AU - Diego, J. M.
AU - Pascale, M.
AU - Kavanagh, B. J.
AU - Kelly, P.
AU - Dai, L.
AU - Frye, B.
AU - Broadhurst, T.
N1 - Publisher Copyright:
© J. M. Diego et al. 2022.
PY - 2022/9/1
Y1 - 2022/9/1
N2 - We model the strong lensing effect in the galaxy cluster PSZ1 G311.65-18.48 (z=0.443) with an improved version of the hybrid method WSLAP+. We extend the number of constraints by including the position of critical points, which are combined with the classic positional constraints of the lensed galaxies. We pay special attention to a transient candidate source (Tr) previously discovered in the giant Sunburst arc (z=2.37). Our lens model predicts Tr to be within a fraction of an arcsecond from the critical curve, which has a larger magnification factor than previously found, but still not large enough to explain the observed flux and lack of counterimages. Possible candidate counterimages are discussed that would lower the magnification required to explain Tr, but extreme magnification factors (> 600) are still required, even in that case. The presence of a small mass perturber with a mass comparable to a dwarf galaxy (M108M) near the position of Tr is needed in order to explain the required magnification and morphology of the lensed galaxy. We discuss how the existence of this perturber could potentially be used to constrain models of dark matter. The large apparent brightness and unresolved nature of the magnified object implies a combination of extreme magnification and a very luminous and compact source (ralt;0.4 pc). Possible candidates are discussed, including an hyperluminous star, a small group of stars, or an accretion disk around a relatively small supermassive black hole (SMBH). Based on spectral information and flux requirements, we argue that a luminous blue variable (LBV) star caught during an outburst is the most likely candidate. Owing to the extreme magnification and luminosity of this source, we dub it Godzilla.
AB - We model the strong lensing effect in the galaxy cluster PSZ1 G311.65-18.48 (z=0.443) with an improved version of the hybrid method WSLAP+. We extend the number of constraints by including the position of critical points, which are combined with the classic positional constraints of the lensed galaxies. We pay special attention to a transient candidate source (Tr) previously discovered in the giant Sunburst arc (z=2.37). Our lens model predicts Tr to be within a fraction of an arcsecond from the critical curve, which has a larger magnification factor than previously found, but still not large enough to explain the observed flux and lack of counterimages. Possible candidate counterimages are discussed that would lower the magnification required to explain Tr, but extreme magnification factors (> 600) are still required, even in that case. The presence of a small mass perturber with a mass comparable to a dwarf galaxy (M108M) near the position of Tr is needed in order to explain the required magnification and morphology of the lensed galaxy. We discuss how the existence of this perturber could potentially be used to constrain models of dark matter. The large apparent brightness and unresolved nature of the magnified object implies a combination of extreme magnification and a very luminous and compact source (ralt;0.4 pc). Possible candidates are discussed, including an hyperluminous star, a small group of stars, or an accretion disk around a relatively small supermassive black hole (SMBH). Based on spectral information and flux requirements, we argue that a luminous blue variable (LBV) star caught during an outburst is the most likely candidate. Owing to the extreme magnification and luminosity of this source, we dub it Godzilla.
KW - Dark matter
KW - Gravitational lensing: strong
KW - Stars: variables: general
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U2 - 10.1051/0004-6361/202243605
DO - 10.1051/0004-6361/202243605
M3 - Article
AN - SCOPUS:85139159376
SN - 0004-6361
VL - 665
JO - Astronomy and astrophysics
JF - Astronomy and astrophysics
M1 - A134
ER -