Study of a slice at +9° to +15° of declination. I. The neutral hydrogen content of galaxies in loose groups

M. A.G. Maia; C. N.A. Willmer; L. N. Da Costa

doi:10.1086/300184

Study of a slice at +9° to +15° of declination. I. The neutral hydrogen content of galaxies in loose groups

M. A.G. Maia
, C. N.A. Willmer
, L. N. Da Costa

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

5 Scopus citations

Abstract

We examine the H I content of spiral galaxies in groups by using a catalog of loose groups of galaxies identified in a magnitude-limited sample (m_z ≤ 15.7) spanning the range 8^h ≤ α ≤ 18^h in right ascension and +9° ≤ δ ≤ +15° in declination. The redshift completeness of the galaxy sample is approximately 95%. No significant effect of H I depletion is found, although there may be a hint that the earliest type spirals are slightly deficient.

Original language	English (US)
Pages (from-to)	49-54
Number of pages	6
Journal	Astronomical Journal
Volume	115
Issue number	1
DOIs	https://doi.org/10.1086/300184
State	Published - Jan 1998
Externally published	Yes

Keywords

Galaxies: clusters: general
ISM: atoms

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.1086/300184

Cite this

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abstract = "We examine the H I content of spiral galaxies in groups by using a catalog of loose groups of galaxies identified in a magnitude-limited sample (mz ≤ 15.7) spanning the range 8h ≤ α ≤ 18h in right ascension and +9° ≤ δ ≤ +15° in declination. The redshift completeness of the galaxy sample is approximately 95\%. No significant effect of H I depletion is found, although there may be a hint that the earliest type spirals are slightly deficient.",

keywords = "Galaxies: clusters: general, ISM: atoms",

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year = "1998",

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AU - Maia, M. A.G.

AU - Willmer, C. N.A.

AU - Da Costa, L. N.

PY - 1998/1

Y1 - 1998/1

N2 - We examine the H I content of spiral galaxies in groups by using a catalog of loose groups of galaxies identified in a magnitude-limited sample (mz ≤ 15.7) spanning the range 8h ≤ α ≤ 18h in right ascension and +9° ≤ δ ≤ +15° in declination. The redshift completeness of the galaxy sample is approximately 95%. No significant effect of H I depletion is found, although there may be a hint that the earliest type spirals are slightly deficient.

AB - We examine the H I content of spiral galaxies in groups by using a catalog of loose groups of galaxies identified in a magnitude-limited sample (mz ≤ 15.7) spanning the range 8h ≤ α ≤ 18h in right ascension and +9° ≤ δ ≤ +15° in declination. The redshift completeness of the galaxy sample is approximately 95%. No significant effect of H I depletion is found, although there may be a hint that the earliest type spirals are slightly deficient.

KW - Galaxies: clusters: general

KW - ISM: atoms

UR - https://www.scopus.com/pages/publications/0008611335

UR - https://www.scopus.com/pages/publications/0008611335#tab=citedBy

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JF - Astronomical Journal

IS - 1

ER -

Study of a slice at +9° to +15° of declination. I. The neutral hydrogen content of galaxies in loose groups

Abstract

Keywords

ASJC Scopus subject areas

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