Infrared polarimetry of the reflection nebula near L 1551 IRS 5

T. Nagata; T. Yamashita; S. Sato; H. Suzuki; J. Hough; R. Garden; I. Gatley

Infrared polarimetry of the reflection nebula near L 1551 IRS 5

T. Nagata, T. Yamashita, S. Sato, H. Suzuki, J. Hough, R. Garden, I. Gatley

Centre for Astrophysics Research (CAR)

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

3 Citations (Scopus)

Abstract

The K-band polarization has been measured in the region extending 30 arcsec to the SW of L 1551 IRS 5. The degree of polarization is exceptionally high, reaching ≡67 per cent. The large polarizations and the azimuthal pattern of the position angles are attributed to scattering of infrared radiation from IRS 5 by dust grains. The infrared brightness distribution resembles that of the optical nebulosity. The authors propose that infrared scattering occurs at the 'walls' of a cavity formed by the interaction of stellar winds with the ambient cloud.

Original language	English
Journal	Monthly Notices of the Royal Astronomical Society
Volume	223
Issue number	1
Publication status	Published - 1986

Cite this

@article{53ed6bceed834f61bfa4121299d8f11f,

title = "Infrared polarimetry of the reflection nebula near L 1551 IRS 5",

abstract = "The K-band polarization has been measured in the region extending 30 arcsec to the SW of L 1551 IRS 5. The degree of polarization is exceptionally high, reaching ≡67 per cent. The large polarizations and the azimuthal pattern of the position angles are attributed to scattering of infrared radiation from IRS 5 by dust grains. The infrared brightness distribution resembles that of the optical nebulosity. The authors propose that infrared scattering occurs at the 'walls' of a cavity formed by the interaction of stellar winds with the ambient cloud.",

author = "T. Nagata and T. Yamashita and S. Sato and H. Suzuki and J. Hough and R. Garden and I. Gatley",

note = "Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society [Full text of this article is not available in the UHRA]",

year = "1986",

language = "English",

volume = "223",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Oxford University Press (OUP)",

number = "1",

}

TY - JOUR

T1 - Infrared polarimetry of the reflection nebula near L 1551 IRS 5

AU - Nagata, T.

AU - Yamashita, T.

AU - Sato, S.

AU - Suzuki, H.

AU - Hough, J.

AU - Garden, R.

AU - Gatley, I.

N1 - Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society [Full text of this article is not available in the UHRA]

PY - 1986

Y1 - 1986

N2 - The K-band polarization has been measured in the region extending 30 arcsec to the SW of L 1551 IRS 5. The degree of polarization is exceptionally high, reaching ≡67 per cent. The large polarizations and the azimuthal pattern of the position angles are attributed to scattering of infrared radiation from IRS 5 by dust grains. The infrared brightness distribution resembles that of the optical nebulosity. The authors propose that infrared scattering occurs at the 'walls' of a cavity formed by the interaction of stellar winds with the ambient cloud.

AB - The K-band polarization has been measured in the region extending 30 arcsec to the SW of L 1551 IRS 5. The degree of polarization is exceptionally high, reaching ≡67 per cent. The large polarizations and the azimuthal pattern of the position angles are attributed to scattering of infrared radiation from IRS 5 by dust grains. The infrared brightness distribution resembles that of the optical nebulosity. The authors propose that infrared scattering occurs at the 'walls' of a cavity formed by the interaction of stellar winds with the ambient cloud.

M3 - Article

SN - 0035-8711

VL - 223

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 1

ER -

Infrared polarimetry of the reflection nebula near L 1551 IRS 5

Abstract

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