The host galaxy of the broad absorption line QSO PG 1700 + 518 and its ring galaxy companion: Nicmos 1.6 micron imaging

Dean C. Hines; Frank J. Low; Rodger I. Thompson; Ray J. Weymann; Lisa J. Storrie-Lombardi

doi:10.1086/306773

The host galaxy of the broad absorption line QSO PG 1700 + 518 and its ring galaxy companion: Nicmos 1.6 micron imaging

Dean C. Hines
, Frank J. Low
, Rodger I. Thompson
, Ray J. Weymann
, Lisa J. Storrie-Lombardi

Astronomy

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

22 Scopus citations

Abstract

The 1.6 μm Near Infrared Camera and Multiobject Spectrometer image of the broad absorption line QSO PG 1700 + 518 clearly resolves the QSO host galaxy and a ringlike companion. The companion is most likely a ring galaxy produced in a collision with the QSO galaxy ∼5 x 10⁷ yr ago. The morphology of the PG 1700 + 518 system is very similar to IRAS 04505-2958 (Boyce et al. 1996). Both objects were identified in a sample of eight QSOs selected by "warm" far-IR colors and extreme IR luminosities (Low et al. 1988). All eight QSOs show signs of strong interaction, and the presence of two head-on colliding systems in this sample may suggest that small impact parameters favor the energizing of IR-luminous QSOs.

Original language	English (US)
Pages (from-to)	140-144
Number of pages	5
Journal	Astrophysical Journal
Volume	512
Issue number	1 PART 1
DOIs	https://doi.org/10.1086/306773
State	Published - Feb 10 1999

Keywords

Galaxies: peculiar
Infrared: galaxies

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.1086/306773

Cite this

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title = "The host galaxy of the broad absorption line QSO PG 1700 + 518 and its ring galaxy companion: Nicmos 1.6 micron imaging",

abstract = "The 1.6 μm Near Infrared Camera and Multiobject Spectrometer image of the broad absorption line QSO PG 1700 + 518 clearly resolves the QSO host galaxy and a ringlike companion. The companion is most likely a ring galaxy produced in a collision with the QSO galaxy ∼5 x 107 yr ago. The morphology of the PG 1700 + 518 system is very similar to IRAS 04505-2958 (Boyce et al. 1996). Both objects were identified in a sample of eight QSOs selected by {"}warm{"} far-IR colors and extreme IR luminosities (Low et al. 1988). All eight QSOs show signs of strong interaction, and the presence of two head-on colliding systems in this sample may suggest that small impact parameters favor the energizing of IR-luminous QSOs.",

keywords = "Galaxies: peculiar, Infrared: galaxies",

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year = "1999",

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T1 - The host galaxy of the broad absorption line QSO PG 1700 + 518 and its ring galaxy companion

T2 - Nicmos 1.6 micron imaging

AU - Hines, Dean C.

AU - Low, Frank J.

AU - Thompson, Rodger I.

AU - Weymann, Ray J.

AU - Storrie-Lombardi, Lisa J.

PY - 1999/2/10

Y1 - 1999/2/10

N2 - The 1.6 μm Near Infrared Camera and Multiobject Spectrometer image of the broad absorption line QSO PG 1700 + 518 clearly resolves the QSO host galaxy and a ringlike companion. The companion is most likely a ring galaxy produced in a collision with the QSO galaxy ∼5 x 107 yr ago. The morphology of the PG 1700 + 518 system is very similar to IRAS 04505-2958 (Boyce et al. 1996). Both objects were identified in a sample of eight QSOs selected by "warm" far-IR colors and extreme IR luminosities (Low et al. 1988). All eight QSOs show signs of strong interaction, and the presence of two head-on colliding systems in this sample may suggest that small impact parameters favor the energizing of IR-luminous QSOs.

AB - The 1.6 μm Near Infrared Camera and Multiobject Spectrometer image of the broad absorption line QSO PG 1700 + 518 clearly resolves the QSO host galaxy and a ringlike companion. The companion is most likely a ring galaxy produced in a collision with the QSO galaxy ∼5 x 107 yr ago. The morphology of the PG 1700 + 518 system is very similar to IRAS 04505-2958 (Boyce et al. 1996). Both objects were identified in a sample of eight QSOs selected by "warm" far-IR colors and extreme IR luminosities (Low et al. 1988). All eight QSOs show signs of strong interaction, and the presence of two head-on colliding systems in this sample may suggest that small impact parameters favor the energizing of IR-luminous QSOs.

KW - Galaxies: peculiar

KW - Infrared: galaxies

UR - https://www.scopus.com/pages/publications/0033540573

UR - https://www.scopus.com/pages/publications/0033540573#tab=citedBy

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SN - 0004-637X

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JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1 PART 1

ER -

The host galaxy of the broad absorption line QSO PG 1700 + 518 and its ring galaxy companion: Nicmos 1.6 micron imaging

Abstract

Keywords

ASJC Scopus subject areas

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