Hubble Space Telescope imaging of the BL lacertae object OJ 287

Research output: Contribution to journalArticle

10 Citations (Scopus)

Abstract

Hubble Space Telescope WFPC-2 I-band (F814W) images of the BL Lacertae object OJ 287 and the surrounding field are presented. We find evidence of associated extended nebulosity near OJ 287, as well as a small nebulosity to the west, which may be spatially coincident with the position of previously observed radio emission. The brightness of a host galaxy is difficult to determine because of the brightness of the active nucleus, but it lies in the range -21.5 > MR > -23.1 (H0 = 100 km s-1 Mpc-1, q0 = 0). No evidence is seen for the previously reported optical "jet" at position angle 220° to a surface brightness limit of I = 24.3 mag arcsec-2. There are several resolved and unresolved objects within 17″ of OJ 287 in the field to limits of / = 25 (point source 5 σ detections). The magnitudes and relative positions of these objects are reported. An offset in the centroid position between the OJ 287 point source and the underlying nebulosity reported by Wurtz, Stocke, and Yee is confirmed and measured to be about 0″.4 (1.2 h-1 kpc at the redshift of OJ 287). This offset is tentatively interpreted as evidence for recent merger activity rather than as a sign of gravitational microlensing.

Original languageEnglish (US)
JournalAstrophysical Journal
Volume484
Issue number2 PART II
StatePublished - 1997

Fingerprint

BL Lacertae objects
Hubble Space Telescope
point source
brightness
merger
point sources
radio
radio emission
centroids
galaxies
nuclei
detection

Keywords

  • BL Lacertae objects: individual (OJ 287)
  • Galaxies: active
  • Galaxies: jets
  • Galaxies: photometry

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Hubble Space Telescope imaging of the BL lacertae object OJ 287. / Yanny, Brian; Jannuzi, Buell Tomasson; Impey, Christopher D.

In: Astrophysical Journal, Vol. 484, No. 2 PART II, 1997.

Research output: Contribution to journalArticle

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abstract = "Hubble Space Telescope WFPC-2 I-band (F814W) images of the BL Lacertae object OJ 287 and the surrounding field are presented. We find evidence of associated extended nebulosity near OJ 287, as well as a small nebulosity to the west, which may be spatially coincident with the position of previously observed radio emission. The brightness of a host galaxy is difficult to determine because of the brightness of the active nucleus, but it lies in the range -21.5 > MR > -23.1 (H0 = 100 km s-1 Mpc-1, q0 = 0). No evidence is seen for the previously reported optical {"}jet{"} at position angle 220° to a surface brightness limit of I = 24.3 mag arcsec-2. There are several resolved and unresolved objects within 17″ of OJ 287 in the field to limits of / = 25 (point source 5 σ detections). The magnitudes and relative positions of these objects are reported. An offset in the centroid position between the OJ 287 point source and the underlying nebulosity reported by Wurtz, Stocke, and Yee is confirmed and measured to be about 0″.4 (1.2 h-1 kpc at the redshift of OJ 287). This offset is tentatively interpreted as evidence for recent merger activity rather than as a sign of gravitational microlensing.",
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T1 - Hubble Space Telescope imaging of the BL lacertae object OJ 287

AU - Yanny, Brian

AU - Jannuzi, Buell Tomasson

AU - Impey, Christopher D

PY - 1997

Y1 - 1997

N2 - Hubble Space Telescope WFPC-2 I-band (F814W) images of the BL Lacertae object OJ 287 and the surrounding field are presented. We find evidence of associated extended nebulosity near OJ 287, as well as a small nebulosity to the west, which may be spatially coincident with the position of previously observed radio emission. The brightness of a host galaxy is difficult to determine because of the brightness of the active nucleus, but it lies in the range -21.5 > MR > -23.1 (H0 = 100 km s-1 Mpc-1, q0 = 0). No evidence is seen for the previously reported optical "jet" at position angle 220° to a surface brightness limit of I = 24.3 mag arcsec-2. There are several resolved and unresolved objects within 17″ of OJ 287 in the field to limits of / = 25 (point source 5 σ detections). The magnitudes and relative positions of these objects are reported. An offset in the centroid position between the OJ 287 point source and the underlying nebulosity reported by Wurtz, Stocke, and Yee is confirmed and measured to be about 0″.4 (1.2 h-1 kpc at the redshift of OJ 287). This offset is tentatively interpreted as evidence for recent merger activity rather than as a sign of gravitational microlensing.

AB - Hubble Space Telescope WFPC-2 I-band (F814W) images of the BL Lacertae object OJ 287 and the surrounding field are presented. We find evidence of associated extended nebulosity near OJ 287, as well as a small nebulosity to the west, which may be spatially coincident with the position of previously observed radio emission. The brightness of a host galaxy is difficult to determine because of the brightness of the active nucleus, but it lies in the range -21.5 > MR > -23.1 (H0 = 100 km s-1 Mpc-1, q0 = 0). No evidence is seen for the previously reported optical "jet" at position angle 220° to a surface brightness limit of I = 24.3 mag arcsec-2. There are several resolved and unresolved objects within 17″ of OJ 287 in the field to limits of / = 25 (point source 5 σ detections). The magnitudes and relative positions of these objects are reported. An offset in the centroid position between the OJ 287 point source and the underlying nebulosity reported by Wurtz, Stocke, and Yee is confirmed and measured to be about 0″.4 (1.2 h-1 kpc at the redshift of OJ 287). This offset is tentatively interpreted as evidence for recent merger activity rather than as a sign of gravitational microlensing.

KW - BL Lacertae objects: individual (OJ 287)

KW - Galaxies: active

KW - Galaxies: jets

KW - Galaxies: photometry

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