Dust grain growth in the interstellar medium of 5 < z < 6.5 quasars

Michal Michalowski; E. Murphy; Jens Hjorth; Darach Jafar Watson; C. Gall; J. S. Dunlop

doi:10.1051/0004-6361/201014902

Dust grain growth in the interstellar medium of 5 < z < 6.5 quasars

Michal Michalowski, E. Murphy, Jens Hjorth, Darach Jafar Watson, C. Gall, J. S. Dunlop

88 Citationer (Scopus)

Abstract

Aims. We investigate whether stellar dust sources i.e. asymptotic giant branch (AGB) stars and supernovae (SNe) can account for dust detected in 5 < z < 6.5 quasars (QSOs). Methods. We calculate the required dust yields per AGB star and per SN using the dust masses of QSOs inferred from their millimeter emission and stellar masses approximated as the difference between the dynamical and the H₂ gas masses of these objects. Results. We find that AGB stars are not efficient enough to form dust in the majority of the z > 5 QSOs, whereas SNe may be able to account for dust in some QSOs. However, they require very high dust yields even for a top-heavy initial mass function. Conclusions. This suggests additional non-stellar dust formation mechanism e.g. significant dust grain growth in the interstellar medium of at least three out of nine z > 5 QSOs. SNe (but not AGB stars) may deliver enough heavy elements to fuel this growth.

Originalsprog	Engelsk
Tidsskrift	Astronomy & Astrophysics
Vol/bind	522
Udgave nummer	A15
Antal sider	5
ISSN	0004-6361
DOI	https://doi.org/10.1051/0004-6361/201014902
Status	Udgivet - 27 okt. 2010

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10.1051/0004-6361/201014902

Citationsformater

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title = "Dust grain growth in the interstellar medium of 5 < z < 6.5 quasars",

abstract = "Aims. We investigate whether stellar dust sources i.e. asymptotic giant branch (AGB) stars and supernovae (SNe) can account for dust detected in 5 < z < 6.5 quasars (QSOs). Methods. We calculate the required dust yields per AGB star and per SN using the dust masses of QSOs inferred from their millimeter emission and stellar masses approximated as the difference between the dynamical and the H2 gas masses of these objects. Results. We find that AGB stars are not efficient enough to form dust in the majority of the z > 5 QSOs, whereas SNe may be able to account for dust in some QSOs. However, they require very high dust yields even for a top-heavy initial mass function. Conclusions. This suggests additional non-stellar dust formation mechanism e.g. significant dust grain growth in the interstellar medium of at least three out of nine z > 5 QSOs. SNe (but not AGB stars) may deliver enough heavy elements to fuel this growth.",

author = "Michal Michalowski and E. Murphy and Jens Hjorth and Watson, {Darach Jafar} and C. Gall and Dunlop, {J. S.}",

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doi = "10.1051/0004-6361/201014902",

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journal = "Astronomy and Astrophysics Supplement Series",

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TY - JOUR

T1 - Dust grain growth in the interstellar medium of 5 < z < 6.5 quasars

AU - Michalowski, Michal

AU - Murphy, E.

AU - Hjorth, Jens

AU - Watson, Darach Jafar

AU - Gall, C.

AU - Dunlop, J. S.

PY - 2010/10/27

Y1 - 2010/10/27

N2 - Aims. We investigate whether stellar dust sources i.e. asymptotic giant branch (AGB) stars and supernovae (SNe) can account for dust detected in 5 < z < 6.5 quasars (QSOs). Methods. We calculate the required dust yields per AGB star and per SN using the dust masses of QSOs inferred from their millimeter emission and stellar masses approximated as the difference between the dynamical and the H2 gas masses of these objects. Results. We find that AGB stars are not efficient enough to form dust in the majority of the z > 5 QSOs, whereas SNe may be able to account for dust in some QSOs. However, they require very high dust yields even for a top-heavy initial mass function. Conclusions. This suggests additional non-stellar dust formation mechanism e.g. significant dust grain growth in the interstellar medium of at least three out of nine z > 5 QSOs. SNe (but not AGB stars) may deliver enough heavy elements to fuel this growth.

AB - Aims. We investigate whether stellar dust sources i.e. asymptotic giant branch (AGB) stars and supernovae (SNe) can account for dust detected in 5 < z < 6.5 quasars (QSOs). Methods. We calculate the required dust yields per AGB star and per SN using the dust masses of QSOs inferred from their millimeter emission and stellar masses approximated as the difference between the dynamical and the H2 gas masses of these objects. Results. We find that AGB stars are not efficient enough to form dust in the majority of the z > 5 QSOs, whereas SNe may be able to account for dust in some QSOs. However, they require very high dust yields even for a top-heavy initial mass function. Conclusions. This suggests additional non-stellar dust formation mechanism e.g. significant dust grain growth in the interstellar medium of at least three out of nine z > 5 QSOs. SNe (but not AGB stars) may deliver enough heavy elements to fuel this growth.

U2 - 10.1051/0004-6361/201014902

DO - 10.1051/0004-6361/201014902

M3 - Journal article

SN - 0004-6361

VL - 522

JO - Astronomy and Astrophysics Supplement Series

JF - Astronomy and Astrophysics Supplement Series

IS - A15

ER -

Dust grain growth in the interstellar medium of 5 < z < 6.5 quasars

Abstract

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