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Galactic Ambient of Host Galaxies of GRBs

Published online by Cambridge University Press:  30 October 2019

Santiago Bernal
Affiliation:
Instituto Espacial Ecuatoriano, PBX: 3801460, Oe5-61, Quito, Ecuador email: [email protected]
Nicolás Vásquez
Affiliation:
Escuela Politécnica Nacional, Box 17-01-2759, E11-253, Quito, Ecuador email: [email protected]
Fiona Hoyle
Affiliation:
Academia Cotopaxi, Box 17-11-6510, De las Higuerrillas y Alondras, Quito, Ecuador email: [email protected]
Jaime Calderón
Affiliation:
Red Cedia, The University of Edinburgh email: [email protected]
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Abstract

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We studied a sample of 1672 galaxies in regions where a GRB event had occurred, in order to determine if the galactic environment plays a significant role on these energetic events. The Luminosity Function distribution for these galaxies shows some interesting features. For instance, there is a decline on the Luminosity Function at Mr~ −20.5; a lack of flatness at Mr~ −14 and higher-than-expected values of Φ(Mr) for Mr < 22.5. A comparison between our data and the Void, Wall and Early galaxies Luminosity Function was performed.

Type
Contributed Papers
Copyright
© International Astronomical Union 2019 

References

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