Infrared observations of high galactic latitude early-type stars

A. Fitzsimmons; F. P. Keenan; E. S. Conlon; P. L. Dufton; P. M. Williams

Infrared observations of high galactic latitude early-type stars

A. Fitzsimmons, F. P. Keenan, E. S. Conlon, P. L. Dufton, P. M. Williams

School of Mathematics and Physics

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

2 Citations (Scopus)

Abstract

Infrared photometry of four relatively faint (8.5 ≤ V ≤ 11.0) early-type stars at high galactic latitude has been made in the J, H, K, L' and narrow-band M wavelengths. This has been combined with previously published ultraviolet and visible observations to enable a comparison with LTE model atmosphere fluxes. The results imply that at least three of the stars are normal main-sequence B-stars at large distances from the galactic plane.

Original language	English
Pages (from-to)	336-338
Number of pages	3
Journal	Monthly Notices of the Royal Astronomical Society
Volume	249
Issue number	2
Publication status	Published - 01 Jan 1991

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

Cite this

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title = "Infrared observations of high galactic latitude early-type stars",

abstract = "Infrared photometry of four relatively faint (8.5 ≤ V ≤ 11.0) early-type stars at high galactic latitude has been made in the J, H, K, L' and narrow-band M wavelengths. This has been combined with previously published ultraviolet and visible observations to enable a comparison with LTE model atmosphere fluxes. The results imply that at least three of the stars are normal main-sequence B-stars at large distances from the galactic plane.",

author = "A. Fitzsimmons and Keenan, \{F. P.\} and Conlon, \{E. S.\} and Dufton, \{P. L.\} and Williams, \{P. M.\}",

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AU - Keenan, F. P.

AU - Conlon, E. S.

AU - Dufton, P. L.

AU - Williams, P. M.

PY - 1991/1/1

Y1 - 1991/1/1

N2 - Infrared photometry of four relatively faint (8.5 ≤ V ≤ 11.0) early-type stars at high galactic latitude has been made in the J, H, K, L' and narrow-band M wavelengths. This has been combined with previously published ultraviolet and visible observations to enable a comparison with LTE model atmosphere fluxes. The results imply that at least three of the stars are normal main-sequence B-stars at large distances from the galactic plane.

AB - Infrared photometry of four relatively faint (8.5 ≤ V ≤ 11.0) early-type stars at high galactic latitude has been made in the J, H, K, L' and narrow-band M wavelengths. This has been combined with previously published ultraviolet and visible observations to enable a comparison with LTE model atmosphere fluxes. The results imply that at least three of the stars are normal main-sequence B-stars at large distances from the galactic plane.

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M3 - Article

AN - SCOPUS:4243910592

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JF - Monthly Notices of the Royal Astronomical Society

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Infrared observations of high galactic latitude early-type stars

Abstract

ASJC Scopus subject areas

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