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The SMA CO(2-1) B0DEGA Legacy Project / B0DEGA Sample

The SMA CO(2-1) B0DEGA Legacy Project. Understanding the connection between detailed molecular gas properties, star formation, nuclear activity and environment in galaxies have so far lacked of statistical significance, specially due to the large number of internal variables driving secular evolution that have to be further combined with external effects. In a pilot study we have succesfully detected CO(2-1) for 30 of these galaxies with the SMA. Based on a design by spyka webmaster.

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The SMA CO(2-1) B0DEGA Legacy Project / B0DEGA Sample | b0dega.iaa.es Reviews

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The SMA CO(2-1) B0DEGA Legacy Project. Understanding the connection between detailed molecular gas properties, star formation, nuclear activity and environment in galaxies have so far lacked of statistical significance, specially due to the large number of internal variables driving secular evolution that have to be further combined with external effects. In a pilot study we have succesfully detected CO(2-1) for 30 of these galaxies with the SMA. Based on a design by spyka webmaster.

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The SMA CO(2-1) B0DEGA Legacy Project / B0DEGA Sample | b0dega.iaa.es Reviews

https://b0dega.iaa.es

The SMA CO(2-1) B0DEGA Legacy Project. Understanding the connection between detailed molecular gas properties, star formation, nuclear activity and environment in galaxies have so far lacked of statistical significance, specially due to the large number of internal variables driving secular evolution that have to be further combined with external effects. In a pilot study we have succesfully detected CO(2-1) for 30 of these galaxies with the SMA. Based on a design by spyka webmaster.

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Publications & Talks / B0DEGA Sample

http://b0dega.iaa.es/publications

AUTHORS: Espada, D. on behalf of the B0DEGA team. TITLE: SMA CO(2-1) B0DEGA Legacy Project. MEETING: Millimeter and Submillimeter Astronomy at High Angular Resolution. PLACE: Academia Sinica, Taipei, Taiwan. AUTHORS: Espada, D. on behalf of the B0DEGA team. TITLE: SMA CO(2-1) B0DEGA Legacy Project. MEETING: SMA Science Symposium. PLACE: CfA, Cambridge, USA. AUTHORS: Espada, D. on behalf of the AMIGA and B0DEGA team. TITLE: Studying galaxy evolution in isolated galaxies with ALMA. DATE: 11-13 February 2009.

2

About B0DEGA / B0DEGA Sample

http://b0dega.iaa.es/about

We present the SMA B0DEGA (Below 0 DEgree GAlaxies) project, a high resolution (3 arcsec) survey of CO(2-1) (and isotopes) emission of the circumnuclear regions (1 arcmin) of 30 previously unexplored southern nearby galaxies obtained using the Submillimeter Array (SMA). The sample is composed of IR-bright galaxies (2.58 x S60 S100 31.5 Jy) with recession velocities V. Lsun and IR luminosities in the range 10. The detection rate of our observations is 100%. We find total gas masses Mgas = 10. The main aim...

3

/ B0DEGA Sample

http://b0dega.iaa.es/archive

The main aim of the B0DEGA project is to investigate the fundamental properties of molecular gas in the circumnuclear regions and its relation with the environment, star formation and nuclear activity. Based on a design by spyka webmaster.

4

Team / B0DEGA Sample

http://b0dega.iaa.es/team

D Espada (despada (at) cfa. harvard.edu). Harvard-Smithsonian Center for Astrophysics (CfA, USA). Academia Sinica, Institute of Astronomy and Astrophysics (ASIAA, Taiwan) Institute of Astronomy, National Central University (NCU, Taiwan). Instituto de Astrofisica de Andalucia (IAA-CSIC, Spain). Universidad de Granada (Spain). Instituto de Astrofisica de Andalucia (IAA-CSIC, Spain). Based on a design by spyka webmaster.

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The SMA CO(2-1) B0DEGA Legacy Project. Understanding the connection between detailed molecular gas properties, star formation, nuclear activity and environment in galaxies have so far lacked of statistical significance, specially due to the large number of internal variables driving secular evolution that have to be further combined with external effects. In a pilot study we have succesfully detected CO(2-1) for 30 of these galaxies with the SMA. Based on a design by spyka webmaster.

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