CO Emission, Molecular Gas, and Metallicity in Main-sequence Star-forming Galaxies at z ∼ 2.3
Abstract We present observations of CO(3−2) in 13 main-sequence z = 2.0–2.5 star-forming galaxies at log ( M * / M ⊙ ) = 10.2 – 10.6 that span a wide range in metallicity (O/H) based on rest-optical spectroscopy. We find that L CO ( 3 − 2 ) ′ /SFR decreases with decreasing metallicity, implying that...
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Published in | The Astrophysical journal Vol. 942; no. 1; p. 24 |
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Main Authors | , , , , , , , , , , , |
Format | Journal Article |
Language | English |
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01.01.2023
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Abstract | Abstract
We present observations of CO(3−2) in 13 main-sequence
z
= 2.0–2.5 star-forming galaxies at
log
(
M
*
/
M
⊙
)
=
10.2
–
10.6
that span a wide range in metallicity (O/H) based on rest-optical spectroscopy. We find that
L
CO
(
3
−
2
)
′
/SFR decreases with decreasing metallicity, implying that the CO luminosity per unit gas mass is lower in low-metallicity galaxies at
z
∼ 2. We constrain the CO-to-H
2
conversion factor (
α
CO
) and find that
α
CO
inversely correlates with metallicity at
z
∼ 2. We derive molecular gas masses (
M
mol
) and characterize the relations among
M
*
, SFR,
M
mol
, and metallicity. At
z
∼ 2,
M
mol
increases and the molecular gas fraction (
M
mol
/
M
*
) decreases with increasing
M
*
, with a significant secondary dependence on SFR. Galaxies at
z
∼ 2 lie on a near-linear molecular KS law that is well-described by a constant depletion time of 700 Myr. We find that the scatter about the mean SFR−
M
*
, O/H−
M
*
, and
M
mol
−
M
*
relations is correlated such that, at fixed
M
*
,
z
∼ 2 galaxies with larger
M
mol
have higher SFR and lower O/H. We thus confirm the existence of a fundamental metallicity relation at
z
∼ 2, where O/H is inversely correlated with both SFR and
M
mol
at fixed
M
*
. These results suggest that the scatter of the
z
∼ 2 star-forming main sequence, mass–metallicity relation, and
M
mol
–
M
*
relation are primarily driven by stochastic variations in gas inflow rates. We place constraints on the mass loading of galactic outflows and perform a metal budget analysis, finding that massive
z
∼ 2 star-forming galaxies retain only 30% of metals produced, implying that a large mass of metals resides in the circumgalactic medium. |
---|---|
AbstractList | We present observations of CO(3−2) in 13 main-sequence z = 2.0–2.5 star-forming galaxies at log(M*/M⊙)=10.2–10.6 that span a wide range in metallicity (O/H) based on rest-optical spectroscopy. We find that LCO(3−2)′/SFR decreases with decreasing metallicity, implying that the CO luminosity per unit gas mass is lower in low-metallicity galaxies at z ∼ 2. We constrain the CO-to-H2 conversion factor (αCO) and find that αCO inversely correlates with metallicity at z ∼ 2. We derive molecular gas masses (Mmol) and characterize the relations among M*, SFR, Mmol, and metallicity. At z ∼ 2, Mmol increases and the molecular gas fraction (Mmol/M*) decreases with increasing M*, with a significant secondary dependence on SFR. Galaxies at z ∼ 2 lie on a near-linear molecular KS law that is well-described by a constant depletion time of 700 Myr. We find that the scatter about the mean SFR−M*, O/H−M*, and Mmol−M* relations is correlated such that, at fixed M*, z ∼ 2 galaxies with larger Mmol have higher SFR and lower O/H. We thus confirm the existence of a fundamental metallicity relation at z ∼ 2, where O/H is inversely correlated with both SFR and Mmol at fixed M*. These results suggest that the scatter of the z ∼ 2 star-forming main sequence, mass–metallicity relation, and Mmol–M* relation are primarily driven by stochastic variations in gas inflow rates. We place constraints on the mass loading of galactic outflows and perform a metal budget analysis, finding that massive z ∼ 2 star-forming galaxies retain only 30% of metals produced, implying that a large mass of metals resides in the circumgalactic medium. Abstract We present observations of CO(3−2) in 13 main-sequence z = 2.0–2.5 star-forming galaxies at log ( M * / M ⊙ ) = 10.2 – 10.6 that span a wide range in metallicity (O/H) based on rest-optical spectroscopy. We find that L CO ( 3 − 2 ) ′ /SFR decreases with decreasing metallicity, implying that the CO luminosity per unit gas mass is lower in low-metallicity galaxies at z ∼ 2. We constrain the CO-to-H 2 conversion factor ( α CO ) and find that α CO inversely correlates with metallicity at z ∼ 2. We derive molecular gas masses ( M mol ) and characterize the relations among M * , SFR, M mol , and metallicity. At z ∼ 2, M mol increases and the molecular gas fraction ( M mol / M * ) decreases with increasing M * , with a significant secondary dependence on SFR. Galaxies at z ∼ 2 lie on a near-linear molecular KS law that is well-described by a constant depletion time of 700 Myr. We find that the scatter about the mean SFR− M * , O/H− M * , and M mol − M * relations is correlated such that, at fixed M * , z ∼ 2 galaxies with larger M mol have higher SFR and lower O/H. We thus confirm the existence of a fundamental metallicity relation at z ∼ 2, where O/H is inversely correlated with both SFR and M mol at fixed M * . These results suggest that the scatter of the z ∼ 2 star-forming main sequence, mass–metallicity relation, and M mol – M * relation are primarily driven by stochastic variations in gas inflow rates. We place constraints on the mass loading of galactic outflows and perform a metal budget analysis, finding that massive z ∼ 2 star-forming galaxies retain only 30% of metals produced, implying that a large mass of metals resides in the circumgalactic medium. We present observations of CO(3−2) in 13 main-sequence z = 2.0–2.5 star-forming galaxies at $\mathrm{log}({M}_{* }/{M}_{\odot })=10.2\mbox{--}10.6$ that span a wide range in metallicity (O/H) based on rest-optical spectroscopy. We find that ${L}_{\mathrm{CO}(3-2)}^{{\prime} }$ /SFR decreases with decreasing metallicity, implying that the CO luminosity per unit gas mass is lower in low-metallicity galaxies at z ∼ 2. We constrain the CO-to-H _2 conversion factor ( α _CO ) and find that α _CO inversely correlates with metallicity at z ∼ 2. We derive molecular gas masses ( M _mol ) and characterize the relations among M _* , SFR, M _mol , and metallicity. At z ∼ 2, M _mol increases and the molecular gas fraction ( M _mol / M _* ) decreases with increasing M _* , with a significant secondary dependence on SFR. Galaxies at z ∼ 2 lie on a near-linear molecular KS law that is well-described by a constant depletion time of 700 Myr. We find that the scatter about the mean SFR− M _* , O/H− M _* , and M _mol − M _* relations is correlated such that, at fixed M _* , z ∼ 2 galaxies with larger M _mol have higher SFR and lower O/H. We thus confirm the existence of a fundamental metallicity relation at z ∼ 2, where O/H is inversely correlated with both SFR and M _mol at fixed M _* . These results suggest that the scatter of the z ∼ 2 star-forming main sequence, mass–metallicity relation, and M _mol – M _* relation are primarily driven by stochastic variations in gas inflow rates. We place constraints on the mass loading of galactic outflows and perform a metal budget analysis, finding that massive z ∼ 2 star-forming galaxies retain only 30% of metals produced, implying that a large mass of metals resides in the circumgalactic medium. |
Author | Kriek, Mariska Davé, Romeel Price, Sedona H. Jones, Tucker Shapley, Alice E. Popping, Gergö Mobasher, Bahram Coil, Alison L. Sanders, Ryan L. Shivaei, Irene Siana, Brian Reddy, Naveen A. |
Author_xml | – sequence: 1 givenname: Ryan L. orcidid: 0000-0003-4792-9119 surname: Sanders fullname: Sanders, Ryan L. – sequence: 2 givenname: Alice E. orcidid: 0000-0003-3509-4855 surname: Shapley fullname: Shapley, Alice E. – sequence: 3 givenname: Tucker orcidid: 0000-0001-5860-3419 surname: Jones fullname: Jones, Tucker – sequence: 4 givenname: Irene orcidid: 0000-0003-4702-7561 surname: Shivaei fullname: Shivaei, Irene – sequence: 5 givenname: Gergö orcidid: 0000-0003-1151-4659 surname: Popping fullname: Popping, Gergö – sequence: 6 givenname: Naveen A. orcidid: 0000-0001-9687-4973 surname: Reddy fullname: Reddy, Naveen A. – sequence: 7 givenname: Romeel orcidid: 0000-0003-2842-9434 surname: Davé fullname: Davé, Romeel – sequence: 8 givenname: Sedona H. orcidid: 0000-0002-0108-4176 surname: Price fullname: Price, Sedona H. – sequence: 9 givenname: Bahram surname: Mobasher fullname: Mobasher, Bahram – sequence: 10 givenname: Mariska orcidid: 0000-0002-7613-9872 surname: Kriek fullname: Kriek, Mariska – sequence: 11 givenname: Alison L. orcidid: 0000-0002-2583-5894 surname: Coil fullname: Coil, Alison L. – sequence: 12 givenname: Brian orcidid: 0000-0002-4935-9511 surname: Siana fullname: Siana, Brian |
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CitedBy_id | crossref_primary_10_1093_mnras_stae777 crossref_primary_10_1093_mnras_stad357 crossref_primary_10_1051_0004_6361_202348661 crossref_primary_10_3847_2041_8213_acb2cf crossref_primary_10_1093_mnras_stae047 crossref_primary_10_1051_0004_6361_202346573 crossref_primary_10_3847_2041_8213_ace619 crossref_primary_10_3847_1538_4357_ad4bd8 crossref_primary_10_3847_1538_4357_aca9cc crossref_primary_10_1051_0004_6361_202347418 crossref_primary_10_1093_mnras_stad3999 crossref_primary_10_3847_1538_4357_acd754 crossref_primary_10_1051_0004_6361_202243817 crossref_primary_10_3847_2041_8213_ace5a0 crossref_primary_10_1093_mnras_stad3345 crossref_primary_10_1051_0004_6361_202346918 crossref_primary_10_1051_0004_6361_202449241 crossref_primary_10_1093_mnras_stad3805 |
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Snippet | Abstract
We present observations of CO(3−2) in 13 main-sequence
z
= 2.0–2.5 star-forming galaxies at
log
(
M
*
/
M
⊙
)
=
10.2
–
10.6
that span a wide range in... We present observations of CO(3−2) in 13 main-sequence z = 2.0–2.5 star-forming galaxies at log(M*/M⊙)=10.2–10.6 that span a wide range in metallicity (O/H)... We present observations of CO(3−2) in 13 main-sequence z = 2.0–2.5 star-forming galaxies at $\mathrm{log}({M}_{* }/{M}_{\odot })=10.2\mbox{--}10.6$ that span a... |
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SubjectTerms | Astrophysics CO line emission Correlation Depletion Galaxies Galaxy evolution High-redshift galaxies Luminosity Main sequence stars Metallicity Molecular gas Molecular gases Scattering Space telescopes Spectroscopy Star formation Stars Stars & galaxies |
Title | CO Emission, Molecular Gas, and Metallicity in Main-sequence Star-forming Galaxies at z ∼ 2.3 |
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