Notes - Instituto de AstrofÃsica de AndalucÃa

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Notes - Instituto de AstrofÃsica de AndalucÃa

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Sites of Violent Star (Ángeles diagram)

elesFormation

Early type

GCs

galaxies

SSCs

ULIRGs

AGN

Interacting

Galaxies

VSF

definition

CNSFRs

Starburst

Nuclei

LBCGs

BCGs

DSph

Full lines: possible connections.

Dashed lines: time evolution.

X-ray Spectra of Seyfert 1 Galaxies X-ray Spectra of Seyfert 1 Galaxies

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Beginning Python - From Novice to Professional

Estudio de la alta atmÃ³sfera de Venus con el instrumento VIRTIS ...

The properties of virialized dark matter halos: signals from the large ...

Sites of Violent Star (Ángeles diagram) elesFormation Early type GCs galaxies SSCs ULIRGs AGN Interacting Galaxies VSF definition CNSFRs Starburst Nuclei LBCGs BCGs DSph Full lines: possible connections. Dashed lines: time evolution.

Page 1 and 2: Research and Training Network on Vi
Page 3 and 4: 11:00 Presentation of participant c
Page 5 and 6: • Germany (U. Fritze von Alvensle
Page 7 and 8: 1- the unique possibility that open
Page 9 and 10: providing a concentration, or focal
Page 11 and 12: - IMF - Mass loss, Z, (binaries) -
Page 13: o Mexico: 1 Do we need to select PI
Page 17 and 18: Summary sketch of key questions - C

Notes - Instituto de AstrofÃ­sica de AndalucÃ­a

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Notes - Instituto de AstrofÃsica de AndalucÃa