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Compact molecular gas emission in local LIRGs among low- and high-z galaxies

  • E. Bellocchi*
  • , M. Pereira-Santaella
  • , L. Colina
  • , A. Labiano
  • , M. Sanchez-Garcia
  • , A. Alonso-Herrero
  • , S. Arribas
  • , S. Garcia-Burillo
  • , M. Villar-Martin
  • , D. Rigopoulou
  • , F. Valentino
  • , A. Puglisi
  • , T. Diaz-Santos
  • , S. Cazzoli
  • , A. Usero
    • *Corresponding author for this work

Research output: Contribution to journal › Journal article › Research › peer-review

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Abstract

We present new CO(2-1) observations of a representative sample of 24 local (z & x2004;

Original languageEnglish
Article numberA60
JournalAstronomy & Astrophysics
Volume664
Number of pages36
ISSN0004-6361
DOIs
Publication statusPublished - 4 Aug 2022

Funding

We thank the anonymous referee for useful comments and suggestions which helped us to improve the quality and presentation of the manuscript. EB and AL acknowledge the support from Comunidad de Madrid through the Atraccion de Talento grant 2017-T1/TIC-5213. This research has been partially funded by the Spanish State Research Agency (AEI) Project MDM-2017-0737 Unidad de Excelencia 'Maria de Maeztu'- Centro de Astrobiologia (INTA-CSIC). MPS acknowledges support from the Comunidad de Madrid through the Atraccion de Talento Investigador Grant 2018-T1/TIC-11035 and PID2019-105423GA-I00 (MCIU/AEI FEDER, UE). AAH, MVM and SGB acknowledge support from grant PGC2018-094671-B-I00 (MCIU/AEI/FEDER,UE). SGB acknowledges support from the research project PID2019-106027GA-C44 of the Spanish Ministerio de Ciencia e Innovacion. DR acknowledges support from STFC through grant ST/S000488/1. AL, LC and SA acknowledge the support from grant PID2019-106280GB-I00 (MCIU/AEI/FEDER,UE). SC acknowledges financial support from the State Agency for Research of the Spanish MCIU through the Center of Excellence Severo Ochoa award to the Instituto de Astrofisica de Andalucia (SEV-2017-0709). MSG acknowledges support from the Spanish Ministerio de Economia y Competitividad through the grants BES-2016-078922 and ESP2017-83197-P. AP gratefully acknowledges financial support from STFC through grant ST/T000244/1. FV acknowledges support from the Carlsberg Foundation Research Grant CF18-0388 'Galaxies: Rise and Death'. The Cosmic Dawn Center (DAWN) is funded by the Danish National Research Foundation under grant No. 140. AU acknowledges support from the Spanish grants PGC2018-094671-B-I00, funded by MCIN/AEI/10.13039/501100011033 and by "ERDF A way of making Europe", and PID2019-108765GB-I00, funded by MCIN/AEI/10.13039/501100011033. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2013.1.00243.S, ADS/JAO.ALMA#2013.1.00271.S, ADS/JAO.ALMA#2015.1.00714.S, ADS/JAO.ALMA#2017.1.00255.S, ADS/JAO.ALMA#2017.1.00395.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), MOST and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ.

Keywords

  • ISM
  • molecules
  • infrared
  • galaxies
  • starburst
  • evolution
  • ULTRALUMINOUS INFRARED GALAXIES
  • INTEGRAL FIELD SPECTROSCOPY
  • STAR-FORMING GALAXIES
  • ACTIVE GALACTIC NUCLEI
  • MASS ASSEMBLY GAMA
  • TO-LIGHT RATIO
  • MAIN-SEQUENCE
  • SUBMILLIMETER GALAXIES
  • ATLAS(3D) PROJECT
  • STELLAR MASS

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