Deep HI imaging of galaxy cluster Abell 2218 at z=0.2

M. Zwaan; P.G.  van Dokkum; MAW Verheijen; F.H. Briggs

Deep HI imaging of galaxy cluster Abell 2218 at z=0.2

M. Zwaan, P.G. van Dokkum, MAW Verheijen, F.H. Briggs

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Academic › peer-review

Abstract

Deep HI imaging with the Westerbork Synthesis Radio Telescope in the direction of Abell 2218 has resulted in the first detection of HI 21 cm emission at cosmological distance. The HI signal originates in a galaxy at a projected distance of 1.5 h(100)(-1) Mpc from the cluster core and is probably in the process of being accreted onto the cluster. The detection of this galaxy demonstrates that HI 21 cm emission line surveys at cosmological distances are feasible with present-day radio telescopes.

Original language	English
Title of host publication	GAS AND GALAXY EVOLUTION: A CONFERENCE IN HONOR OF THE 20TH ANNIVERSARY OF THE VLA
Editors	JE Hibbard, MP Rupen, JH VanGorkom
Place of Publication	SAN FRANCISCO
Publisher	ASTRONOMICAL SOC PACIFIC
Pages	640-641
Number of pages	2
ISBN (Print)	1-58381-077-3
Publication status	Published - 2001
Event	Conference on Gas and Galaxy Evolution in Honor of the 20th Anniversary of the VLA - Duration: 21-May-2000 → 24-May-2000

Publication series

Name	ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES
Publisher	ASTRONOMICAL SOC PACIFIC
Volume	240

Other

Other	Conference on Gas and Galaxy Evolution in Honor of the 20th Anniversary of the VLA
Period	21/05/2000 → 24/05/2000

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@inproceedings{66c9a4d21a1a4bde8a846142a86e8d2e,

title = "Deep HI imaging of galaxy cluster Abell 2218 at z=0.2",

abstract = "Deep HI imaging with the Westerbork Synthesis Radio Telescope in the direction of Abell 2218 has resulted in the first detection of HI 21 cm emission at cosmological distance. The HI signal originates in a galaxy at a projected distance of 1.5 h(100)(-1) Mpc from the cluster core and is probably in the process of being accreted onto the cluster. The detection of this galaxy demonstrates that HI 21 cm emission line surveys at cosmological distances are feasible with present-day radio telescopes.",

author = "M. Zwaan and {van Dokkum}, P.G. and MAW Verheijen and F.H. Briggs",

year = "2001",

language = "English",

isbn = "1-58381-077-3",

series = "ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES",

publisher = "ASTRONOMICAL SOC PACIFIC",

pages = "640--641",

editor = "JE Hibbard and MP Rupen and JH VanGorkom",

booktitle = "GAS AND GALAXY EVOLUTION: A CONFERENCE IN HONOR OF THE 20TH ANNIVERSARY OF THE VLA",

note = "Conference on Gas and Galaxy Evolution in Honor of the 20th Anniversary of the VLA ; Conference date: 21-05-2000 Through 24-05-2000",

}

Zwaan, M, van Dokkum, PG, Verheijen, MAW & Briggs, FH 2001, Deep HI imaging of galaxy cluster Abell 2218 at z=0.2. in JE Hibbard, MP Rupen & JH VanGorkom (eds), GAS AND GALAXY EVOLUTION: A CONFERENCE IN HONOR OF THE 20TH ANNIVERSARY OF THE VLA. ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES, vol. 240, ASTRONOMICAL SOC PACIFIC, SAN FRANCISCO, pp. 640-641, Conference on Gas and Galaxy Evolution in Honor of the 20th Anniversary of the VLA, 21/05/2000.

Deep HI imaging of galaxy cluster Abell 2218 at z=0.2. / Zwaan, M.; van Dokkum, P.G. ; Verheijen, MAW et al.
GAS AND GALAXY EVOLUTION: A CONFERENCE IN HONOR OF THE 20TH ANNIVERSARY OF THE VLA. ed. / JE Hibbard; MP Rupen; JH VanGorkom. SAN FRANCISCO: ASTRONOMICAL SOC PACIFIC, 2001. p. 640-641 (ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES; Vol. 240).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Academic › peer-review

TY - GEN

T1 - Deep HI imaging of galaxy cluster Abell 2218 at z=0.2

AU - Zwaan, M.

AU - van Dokkum, P.G.

AU - Verheijen, MAW

AU - Briggs, F.H.

PY - 2001

Y1 - 2001

N2 - Deep HI imaging with the Westerbork Synthesis Radio Telescope in the direction of Abell 2218 has resulted in the first detection of HI 21 cm emission at cosmological distance. The HI signal originates in a galaxy at a projected distance of 1.5 h(100)(-1) Mpc from the cluster core and is probably in the process of being accreted onto the cluster. The detection of this galaxy demonstrates that HI 21 cm emission line surveys at cosmological distances are feasible with present-day radio telescopes.

AB - Deep HI imaging with the Westerbork Synthesis Radio Telescope in the direction of Abell 2218 has resulted in the first detection of HI 21 cm emission at cosmological distance. The HI signal originates in a galaxy at a projected distance of 1.5 h(100)(-1) Mpc from the cluster core and is probably in the process of being accreted onto the cluster. The detection of this galaxy demonstrates that HI 21 cm emission line surveys at cosmological distances are feasible with present-day radio telescopes.

M3 - Conference contribution

SN - 1-58381-077-3

T3 - ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES

SP - 640

EP - 641

BT - GAS AND GALAXY EVOLUTION: A CONFERENCE IN HONOR OF THE 20TH ANNIVERSARY OF THE VLA

A2 - Hibbard, JE

A2 - Rupen, MP

A2 - VanGorkom, JH

PB - ASTRONOMICAL SOC PACIFIC

CY - SAN FRANCISCO

T2 - Conference on Gas and Galaxy Evolution in Honor of the 20th Anniversary of the VLA

Y2 - 21 May 2000 through 24 May 2000

ER -

Deep HI imaging of galaxy cluster Abell 2218 at z=0.2

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