2024A&A...681A..44S


Query : 2024A&A...681A..44S

2024A&A...681A..44S - Astronomy and Astrophysics, volume 681A44 (2024/1-1)

Tracing Population III supernovae with extreme energies through the Sculptor dwarf spheroidal galaxy.

SKULADOTTIR A., VANNI I., SALVADORI S. and LUCCHESI R.

Abstract (from CDS):

The Sculptor dwarf spheroidal galaxy is old and metal-poor, making it ideal to study the earliest chemical enrichment in the Local Group. We followed up on the most metal-poor star known in this (or any external) galaxy, AS0039, with high-resolution ESO VLT/UVES spectra. Our new analysis confirmed its low metallicity, [Fe/H]LTE = -3.90 ± 0.15, and that it is extremely C-poor, with A(C) = + 3.60, which corresponds to [C/Fe]LTE = -0.33 ± 0.17 (accounting for internal mixing). This adds to the evidence of Sculptor being intrinsically C-poor at low [Fe/H] ≲ -3. However, here we also report a new discovery of a carbon-enhanced metal-poor (CEMP-no) star in Sculptor, DR20080, with no enhancement of Ba, indicative of enrichment by zero-metallicity low-energy supernovae, ESN < 1 × 1051. This is the first piece of evidence of a dual population of CEMP-no and C-normal stars in Sculptor at [Fe/H] ≤ -3. The fraction of CEMP-no stars is still low, $ f^{\mathrm{Scl}}_{\mathrm{CEMP}}=9^{+11}_{-8}\% $ at -4 ≤ [Fe/H] ≤ -3, compared to the significantly higher fraction in the Milky Way halo, $ f^{\mathrm{MW}}_{\mathrm{CEMP}}\approx40\% $. To further investigate the early chemical enrichment of Sculptor, we re-derived chemical abundances of light, α, iron-peak, and neutron-capture elements in all Sculptor stars at [Fe/H] ≤ -2.8, with available high-resolution spectra. Our results show that at these low [Fe/H], Sculptor is deficient in light elements (e.g. C, Na, Al, Mg) relative to both the Milky Way halo, and ultra-faint dwarf galaxies, pointing towards a significant contribution from high-energy supernovae. Furthermore, the abundance pattern of the star AS0039 is best fitted with a zero-metallicity hypernova progenitor, ESN = 10 × 1051, with a mass of M = 20 M⊙. Our results in Sculptor, at [Fe/H] ≤ -3, therefore suggest significant enrichment by both very low-energy supernovae and hypernovae, solidifying this galaxy as one of the benchmarks for understanding the energy distribution of the first supernova in the Universe.

Abstract Copyright: © The Authors 2024

Journal keyword(s): stars: abundances - stars: carbon - stars: chemically peculiar - stars: Population III - galaxies: abundances - galaxies: individual: Sculptor

Simbad objects: 26

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Number of rows : 26
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 2MASS J00571020-3328359 Ev* 00 57 10.2179527464 -33 28 35.800377672   18.765 17.798   16.655 ~ 10 0
2 2MASS J00573485-3339457 Ev* 00 57 34.8471871440 -33 39 45.706787496   19.017 18.058   16.962 ~ 9 0
3 2MASS J00574417-3401139 Ev* 00 57 44.1582595968 -34 01 14.322933588     18.28   17.1 ~ 3 0
4 [MFW2011] 26017 Ev* 00 58 45.5978140704 -33 42 21.787062912           ~ 7 0
5 GB07 Scl49 RG* 00 59 08.6092477128 -33 42 29.639424852     17.975   16.89 ~ 18 0
6 GB07 Scl76 RG* 00 59 12.0972695640 -33 46 20.953491492     17.266 16.36 15.98 ~ 21 0
7 [CSF2018] 11-1-4296 Pe* 00 59 38.7626222568 -33 46 14.631963456     19.16   18.04 ~ 10 0
8 2MASS J00594706-3342543 RG* 00 59 47.0571830400 -33 42 54.294121548     17.810   16.721 ~ 17 0
9 [CSF2018] 6-6-402 Ev* 01 00 00.4077384576 -33 29 15.452889144           ~ 8 0
10 [V78] 551 Ev* 01 00 01.1459036832 -33 59 21.358222944           ~ 13 0
11 NAME Sculptor Dwarf Galaxy G 01 00 09.4 -33 42 32   9.79 8.6 8.81   ~ 1498 4
12 2MASS J01004785-3341029 RG* 01 00 47.8436551872 -33 41 03.185910636   19.16 18.187   17.116 ~ 22 0
13 [MFW2011] 24017 Ev* 01 01 22.2460670952 -33 46 21.849866004           ~ 10 0
14 [SHT2013] Scl002 06 Ev* 01 01 26.7622707600 -33 02 59.802667188   18.265 17.120   15.784 ~ 8 0
15 [CSF2018] 10-8-61 Ev* 01 01 47.4804961320 -33 47 27.568418604   19.482 18.674   17.671 ~ 5 0
16 2MASS J01014944-3354103 LP* 01 01 49.4335266000 -33 54 10.379923560     17.130   15.623 ~ 9 0
17 MCG-06-07-001 G 02 39 59.3 -34 26 57   9.02 7.4     ~ 1894 1
18 NAME Reticulum II G 03 35 42.1 -54 02 57           ~ 375 0
19 ESO 206-20A G 06 41 36.7 -50 57 58   22.14 11.0 19.47   ~ 1190 0
20 NAME Sextans dSph LSB 10 13 02.9 -01 36 53   12 10.4     ~ 921 0
21 NAME Leo IV LSB 11 32 57.0 -00 32 00     15.1     ~ 419 1
22 NAME Bootes II G 13 58 00.0 +12 51 00     15.4     ~ 269 0
23 NAME Hercules Dwarf Galaxy G 16 31 02.0 +12 47 30     14.0     ~ 379 1
24 BPS CS 22892-0052 Pe* 22 17 01.6558764360 -16 39 27.051026544   14.03 13.20 13.06 12.19 KIIvw 472 0
25 NAME Local Group GrG ~ ~           ~ 9325 0
26 NAME Galactic Bulge reg ~ ~           ~ 4794 0

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