期刊
ASTROPHYSICAL JOURNAL
卷 750, 期 2, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/750/2/92
关键词
galaxies: active; galaxies: evolution; galaxies: high-redshift; galaxies: starburst; radio lines: galaxies
资金
- INSU/CNRS (France)
- MPG (Germany)
- IGN (Spain)
- NSF of China [10833006, 10973011, 11003015, 11173059]
- 973 project [2007CB815405]
- Chinese Academy of Sciences
- STFC [ST/J001562/1] Funding Source: UKRI
- Science and Technology Facilities Council [ST/J001562/1] Funding Source: researchfish
We report CO detections in 17 out of 19 infrared ultraluminous QSO (IR QSO) hosts observed with the IRAM 30 m telescope. The cold molecular gas reservoir in these objects is in a range of (0.2-2.1) x 10(10) M-circle dot (adopting a CO-to-H-2 conversion factor alpha CO = 0.8 M-circle dot (K km s(-1) pc(2))(-1)). We find that the molecular gas properties of IR QSOs, such as the molecular gas mass, star formation efficiency (L-FIR/L'(CO)), and CO (1-0) line widths, are indistinguishable from those of local ultraluminous infrared galaxies (ULIRGs). A comparison of low-and high-redshift CO-detected QSOs reveals a tight correlation between L-FIR and L'(CO(1-0)) for all QSOs. This suggests that, similar to ULIRGs, the far-infrared emissions of all QSOs are mainly from dust heated by star formation rather than by active galactic nuclei (AGNs), confirming similar findings from mid-infrared spectroscopic observations by Spitzer. A correlation between the AGN-associated bolometric luminosities and the CO line luminosities suggests that star formation and AGNs draw from the same reservoir of gas and there is a link between star formation on similar to kpc scale and the central black hole accretion process on much smaller scales.
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