Possible depletion of metals into dust grains in the core of
the Centaurus cluster of galaxies

J 2019

Possible depletion of metals into dust grains in the core of the Centaurus cluster of galaxies

LAKHCHAURA, K.; F. MERNIER a Norbert WERNER

Základní údaje

Originální název

Possible depletion of metals into dust grains in the core of the Centaurus cluster of galaxies

Autoři

LAKHCHAURA, K.; F. MERNIER a Norbert WERNER

Vydání

ASTRONOMY & ASTROPHYSICS, LES ULIS CEDEX A, EDP SCIENCES S A, 2019, 0004-6361

Další údaje

Jazyk

angličtina

Typ výsledku

Článek v odborném periodiku

Obor

10308 Astronomy

Stát vydavatele

Francie

Utajení

není předmětem státního či obchodního tajemství

Odkazy

URL, Full Text

Impakt faktor

Impact factor: 5.636

Označené pro přenos do RIV

Ano

Kód RIV

RIV/00216224:14310/19:00109245

Organizační jednotka

Přírodovědecká fakulta

Klíčová slova anglicky

galaxies: abundances; galaxies: evolution; galaxies: active; X-rays: galaxies: clusters

Štítky

rivok

Příznaky

Mezinárodní význam, Recenzováno

Změněno: 10. 11. 2022 12:10, Mgr. Marie Novosadová Šípková, DiS.

Anotace

V originále

We present azimuthally averaged metal abundance profiles from a full, comprehensive, and conservative re-analysis of the deep (similar to 800 ks total net exposure) Chandra/ACIS-S observation of the Centaurus cluster core (NGC 4696). After carefully checking various sources of systematic uncertainties, including the choice of the spectral deprojection method, assumptions about the temperature structure of the gas, and uncertainties in the continuum modeling, we confirm the existence of a central drop in the abundances of the "reactive" elements Fe, Si, S, Mg, and Ca, within r less than or similar to 10 kpc. The same drops are also found when analyzing the XMM-Newton/EPIC data (similar to 150 ks). Adopting our most conservative approach, we find that, unlike the central drops seen for Fe, Si, S, Mg and Ca, the abundance of the "nonreactive" element Ar is fully consistent with showing no central drop. This is further confirmed by the significant (>3 sigma) central radial increase of the Ar/Fe ratio. Our results corroborate the previously proposed "dust depletion scenario", in which central metal abundance drops are explained by the deposition of a significant fraction of centrally cooled reactive metals into dust grains present in the central regions of the Centaurus cluster. This is also supported by the previous findings that the extent of the metal abundance drops in NGC4696 broadly coincides with the infrared dust emission.

Citovat

LAKHCHAURA, K.; F. MERNIER a Norbert WERNER. Possible depletion of metals into dust grains in the core of the Centaurus cluster of galaxies. ASTRONOMY & ASTROPHYSICS. LES ULIS CEDEX A: EDP SCIENCES S A, 2019, roč. 623, č. 17, s. 1-11. ISSN 0004-6361. Dostupné z: https://doi.org/10.1051/0004-6361/201834755.

@article{1504140,
   author = {Lakhchaura, K. and Mernier, F. and Werner, Norbert},
   article_location = {LES ULIS CEDEX A},
   article_number = {17},
   doi = {https://doi.org/10.1051/0004-6361/201834755},
   keywords = {galaxies: abundances; galaxies: evolution; galaxies: active; X-rays: galaxies: clusters},
   language = {eng},
   issn = {0004-6361},
   journal = {ASTRONOMY & ASTROPHYSICS},
   title = {Possible depletion of metals into dust grains in the core of the Centaurus cluster of galaxies},
   url = {https://arxiv.org/pdf/1812.00121.pdf},
   volume = {623},
   year = {2019}
}

TY  - JOUR
ID  - 1504140
AU  - Lakhchaura, K. - Mernier, F. - Werner, Norbert
PY  - 2019
TI  - Possible depletion of metals into dust grains in the core of the Centaurus cluster of galaxies
JF  - ASTRONOMY & ASTROPHYSICS
VL  - 623
IS  - 17
SP  - 1-11
EP  - 1-11
PB  - EDP SCIENCES S A
SN  - 00046361
KW  - galaxies: abundances
KW  - galaxies: evolution
KW  - galaxies: active
KW  - X-rays: galaxies: clusters
UR  - https://arxiv.org/pdf/1812.00121.pdf
N2  - We present azimuthally averaged metal abundance profiles from a full, comprehensive, and conservative re-analysis of the deep (similar to 800 ks total net exposure) Chandra/ACIS-S observation of the Centaurus cluster core (NGC 4696). After carefully checking various sources of systematic uncertainties, including the choice of the spectral deprojection method, assumptions about the temperature structure of the gas, and uncertainties in the continuum modeling, we confirm the existence of a central drop in the abundances of the "reactive" elements Fe, Si, S, Mg, and Ca, within r less than or similar to 10 kpc. The same drops are also found when analyzing the XMM-Newton/EPIC data (similar to 150 ks). Adopting our most conservative approach, we find that, unlike the central drops seen for Fe, Si, S, Mg and Ca, the abundance of the "nonreactive" element Ar is fully consistent with showing no central drop. This is further confirmed by the significant (>3 sigma) central radial increase of the Ar/Fe ratio. Our results corroborate the previously proposed "dust depletion scenario", in which central metal abundance drops are explained by the deposition of a significant fraction of centrally cooled reactive metals into dust grains present in the central regions of the Centaurus cluster. This is also supported by the previous findings that the extent of the metal abundance drops in NGC4696 broadly coincides with the infrared dust emission.
ER  -

LAKHCHAURA, K.; F. MERNIER a Norbert WERNER. Possible depletion of metals into dust grains in the core of the Centaurus cluster of galaxies. \textit{ASTRONOMY \&{} ASTROPHYSICS}. LES ULIS CEDEX A: EDP SCIENCES S A, 2019, roč.~623, č.~17, s.~1-11. ISSN~0004-6361. Dostupné z: https://doi.org/10.1051/0004-6361/201834755.

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