The Hydra-Centaurus region and the nearby universe

C. N.A. Willmer; L. N. Da Costa; P. S. Pellegrini; A. P. Fairall; David W. Latham; Wolfram Freudling

doi:10.1086/117256

The Hydra-Centaurus region and the nearby universe

C. N.A. Willmer, L. N. Da Costa, P. S. Pellegrini, A. P. Fairall, David W. Latham, Wolfram Freudling

Research output: Contribution to journal › Article › peer-review

1 Scopus citations

Abstract

In this paper we present maps of the spatial distribution of galaxies in the general direction of the Hydra-Centaurus complex and discuss how that distribution relates to other structures located in the volume within 6000 km s^-1 of the Local Group, using a sample of over 5700 galaxies brighter than m_B(0) = 14.5 with essentially complete redshift information. Our sample covers about 50% of the sky and allows us to follow structures over large extensions. From the inspection of these maps we find that the galaxies are distributed in a pattern of interconnected structures, many of them with a rather regular wall-like appearance.

Original language	English (US)
Pages (from-to)	61-72
Number of pages	12
Journal	Astronomical Journal
Volume	109
Issue number	1
DOIs	https://doi.org/10.1086/117256
State	Published - Jan 1995
Externally published	Yes

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.1086/117256

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title = "The Hydra-Centaurus region and the nearby universe",

abstract = "In this paper we present maps of the spatial distribution of galaxies in the general direction of the Hydra-Centaurus complex and discuss how that distribution relates to other structures located in the volume within 6000 km s-1 of the Local Group, using a sample of over 5700 galaxies brighter than mB(0) = 14.5 with essentially complete redshift information. Our sample covers about 50% of the sky and allows us to follow structures over large extensions. From the inspection of these maps we find that the galaxies are distributed in a pattern of interconnected structures, many of them with a rather regular wall-like appearance.",

author = "Willmer, {C. N.A.} and {Da Costa}, {L. N.} and Pellegrini, {P. S.} and Fairall, {A. P.} and Latham, {David W.} and Wolfram Freudling",

year = "1995",

month = jan,

doi = "10.1086/117256",

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AU - Willmer, C. N.A.

AU - Da Costa, L. N.

AU - Pellegrini, P. S.

AU - Fairall, A. P.

AU - Latham, David W.

AU - Freudling, Wolfram

PY - 1995/1

Y1 - 1995/1

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AB - In this paper we present maps of the spatial distribution of galaxies in the general direction of the Hydra-Centaurus complex and discuss how that distribution relates to other structures located in the volume within 6000 km s-1 of the Local Group, using a sample of over 5700 galaxies brighter than mB(0) = 14.5 with essentially complete redshift information. Our sample covers about 50% of the sky and allows us to follow structures over large extensions. From the inspection of these maps we find that the galaxies are distributed in a pattern of interconnected structures, many of them with a rather regular wall-like appearance.

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The Hydra-Centaurus region and the nearby universe

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