On the nature of Dwarf Galaxies in the interacting group HCG 31

Angel Lopez Sanchez; Cesar Esteban; Mónica Rodríguez

doi:10.1017/S0074180900198419

On the nature of Dwarf Galaxies in the interacting group HCG 31

Angel Lopez Sanchez, Cesar Esteban, Mónica Rodríguez

Research output: Contribution to journal › Conference paper

Abstract

We have analysed the morphology, kinematics, colors and chemical composition of the ionized gas of the different objects belonging to the interacting compact group HCG 31 in order to get a global view of the origin and evolution of the dwarf galaxies present in it.

Original language	English
Pages (from-to)	568-569
Number of pages	2
Journal	Proceedings of the International Astronomical Union
Volume	217
DOIs	https://doi.org/10.1017/S0074180900198419
Publication status	Published - 2004
Externally published	Yes
Event	217th Symposium of the International-Astronomical-Union on Recycling Intergalactic and Interstellar Matter held at the 25th IAU General Assembly - Sydney, Australia Duration: 6 Aug 2002 → 10 Aug 2002

Access to Document

10.1017/S0074180900198419

Cite this

@article{c96489be01dc43ad872bb776c9d634df,

title = "On the nature of Dwarf Galaxies in the interacting group HCG 31",

abstract = "We have analysed the morphology, kinematics, colors and chemical composition of the ionized gas of the different objects belonging to the interacting compact group HCG 31 in order to get a global view of the origin and evolution of the dwarf galaxies present in it.",

author = "{Lopez Sanchez}, Angel and Cesar Esteban and M{\'o}nica Rodr{\'i}guez",

year = "2004",

doi = "10.1017/S0074180900198419",

language = "English",

volume = "217",

pages = "568--569",

journal = "Proceedings of the International Astronomical Union",

issn = "1743-9213",

publisher = "Cambridge University Press",

}

TY - JOUR

T1 - On the nature of Dwarf Galaxies in the interacting group HCG 31

AU - Lopez Sanchez, Angel

AU - Esteban, Cesar

AU - Rodríguez, Mónica

PY - 2004

Y1 - 2004

N2 - We have analysed the morphology, kinematics, colors and chemical composition of the ionized gas of the different objects belonging to the interacting compact group HCG 31 in order to get a global view of the origin and evolution of the dwarf galaxies present in it.

AB - We have analysed the morphology, kinematics, colors and chemical composition of the ionized gas of the different objects belonging to the interacting compact group HCG 31 in order to get a global view of the origin and evolution of the dwarf galaxies present in it.

U2 - 10.1017/S0074180900198419

DO - 10.1017/S0074180900198419

M3 - Conference paper

VL - 217

SP - 568

EP - 569

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

ER -