The gravitational lens candidate HE 1104-1805 and the size of absorption systems

A Smette; JG Robertson; PA Shaver; D Reimers; L Wisotzki; T Kohler

The gravitational lens candidate HE 1104-1805 and the size of absorption systems

A Smette^*
, JG Robertson
, PA Shaver
, D Reimers
, L Wisotzki
, T Kohler

^*Corresponding author for this work

University of Groningen

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

Abstract

We obtained 1.2 Angstrom resolution spectra over the range 3175 - 7575 Angstrom for the two components of the gravitational lens candidate HE 1104-1805 (z = 2.31, m(B) = 16.7 and 18.6, separation = 3.0 arcsec; cf. Wisotzki et al. 1993), with the aim of setting limits on the sizes of the clouds producing the Ly-alpha, CIV, and MgII absorption systems. We refer to Smette et al. (1995) for a detailed account of this study.

Original language	English
Title of host publication	ASTROPHYSICAL APPLICATIONS OF GRAVITATIONAL LENSING
Editors	CS Kochanek, JN Hewitt
Place of Publication	DORDRECHT
Publisher	Kluwer Academic Publishers
Pages	101-102
Number of pages	2
ISBN (Print)	0-7923-3954-1
Publication status	Published - 1996
Event	173rd Symposium of the International-Astronomical-Union on Astrophysical Applications of Gravitational Lensing - , Australia Duration: 9-Jul-1995 → 14-Jul-1995

Publication series

Name	IAU SYMPOSIA
Publisher	KLUWER ACADEMIC PUBL
ISSN (Print)	0074-1809

Other

Other	173rd Symposium of the International-Astronomical-Union on Astrophysical Applications of Gravitational Lensing
Country/Territory	Australia
Period	09/07/1995 → 14/07/1995

Keywords

QSO

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@inproceedings{d867e00d933846e482a9ff888682064a,

title = "The gravitational lens candidate HE 1104-1805 and the size of absorption systems",

abstract = "We obtained 1.2 Angstrom resolution spectra over the range 3175 - 7575 Angstrom for the two components of the gravitational lens candidate HE 1104-1805 (z = 2.31, m(B) = 16.7 and 18.6, separation = 3.0 arcsec; cf. Wisotzki et al. 1993), with the aim of setting limits on the sizes of the clouds producing the Ly-alpha, CIV, and MgII absorption systems. We refer to Smette et al. (1995) for a detailed account of this study.",

keywords = "QSO",

author = "A Smette and JG Robertson and PA Shaver and D Reimers and L Wisotzki and T Kohler",

year = "1996",

language = "English",

isbn = "0-7923-3954-1",

series = "IAU SYMPOSIA",

publisher = "Kluwer Academic Publishers",

pages = "101--102",

editor = "CS Kochanek and JN Hewitt",

booktitle = "ASTROPHYSICAL APPLICATIONS OF GRAVITATIONAL LENSING",

note = "173rd Symposium of the International-Astronomical-Union on Astrophysical Applications of Gravitational Lensing ; Conference date: 09-07-1995 Through 14-07-1995",

}

Smette, A, Robertson, JG, Shaver, PA, Reimers, D, Wisotzki, L & Kohler, T 1996, The gravitational lens candidate HE 1104-1805 and the size of absorption systems. in CS Kochanek & JN Hewitt (eds), ASTROPHYSICAL APPLICATIONS OF GRAVITATIONAL LENSING. IAU SYMPOSIA, Kluwer Academic Publishers, DORDRECHT, pp. 101-102, 173rd Symposium of the International-Astronomical-Union on Astrophysical Applications of Gravitational Lensing, Australia, 09/07/1995.

The gravitational lens candidate HE 1104-1805 and the size of absorption systems. / Smette, A; Robertson, JG; Shaver, PA et al.
ASTROPHYSICAL APPLICATIONS OF GRAVITATIONAL LENSING. ed. / CS Kochanek; JN Hewitt. DORDRECHT: Kluwer Academic Publishers, 1996. p. 101-102 (IAU SYMPOSIA).

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

TY - GEN

T1 - The gravitational lens candidate HE 1104-1805 and the size of absorption systems

AU - Smette, A

AU - Robertson, JG

AU - Shaver, PA

AU - Reimers, D

AU - Wisotzki, L

AU - Kohler, T

PY - 1996

Y1 - 1996

N2 - We obtained 1.2 Angstrom resolution spectra over the range 3175 - 7575 Angstrom for the two components of the gravitational lens candidate HE 1104-1805 (z = 2.31, m(B) = 16.7 and 18.6, separation = 3.0 arcsec; cf. Wisotzki et al. 1993), with the aim of setting limits on the sizes of the clouds producing the Ly-alpha, CIV, and MgII absorption systems. We refer to Smette et al. (1995) for a detailed account of this study.

AB - We obtained 1.2 Angstrom resolution spectra over the range 3175 - 7575 Angstrom for the two components of the gravitational lens candidate HE 1104-1805 (z = 2.31, m(B) = 16.7 and 18.6, separation = 3.0 arcsec; cf. Wisotzki et al. 1993), with the aim of setting limits on the sizes of the clouds producing the Ly-alpha, CIV, and MgII absorption systems. We refer to Smette et al. (1995) for a detailed account of this study.

KW - QSO

M3 - Conference contribution

SN - 0-7923-3954-1

T3 - IAU SYMPOSIA

SP - 101

EP - 102

BT - ASTROPHYSICAL APPLICATIONS OF GRAVITATIONAL LENSING

A2 - Kochanek, CS

A2 - Hewitt, JN

PB - Kluwer Academic Publishers

CY - DORDRECHT

T2 - 173rd Symposium of the International-Astronomical-Union on Astrophysical Applications of Gravitational Lensing

Y2 - 9 July 1995 through 14 July 1995

ER -

The gravitational lens candidate HE 1104-1805 and the size of absorption systems

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