University of Hertfordshire

By the same authors

Estimating the low-mass IMF in OB associations : o Orionis

Research output: Chapter in Book/Report/Conference proceedingChapter

Standard

Estimating the low-mass IMF in OB associations : o Orionis. / Burningham, B.; Naylor, T.; Littlefair, S.P.; Jefferies, R.D.

The Initial Mass Function 50 Years Later. Springer, 2005. p. 141-142 (Astrophysics and Space Science Library; Vol. 327, No. III).

Research output: Chapter in Book/Report/Conference proceedingChapter

Harvard

Burningham, B, Naylor, T, Littlefair, SP & Jefferies, RD 2005, Estimating the low-mass IMF in OB associations : o Orionis. in The Initial Mass Function 50 Years Later. Astrophysics and Space Science Library, no. III, vol. 327, Springer, pp. 141-142. https://doi.org/10.1007/978-1-4020-3407-7_24

APA

Burningham, B., Naylor, T., Littlefair, S. P., & Jefferies, R. D. (2005). Estimating the low-mass IMF in OB associations : o Orionis. In The Initial Mass Function 50 Years Later (pp. 141-142). (Astrophysics and Space Science Library; Vol. 327, No. III). Springer. https://doi.org/10.1007/978-1-4020-3407-7_24

Vancouver

Burningham B, Naylor T, Littlefair SP, Jefferies RD. Estimating the low-mass IMF in OB associations : o Orionis. In The Initial Mass Function 50 Years Later. Springer. 2005. p. 141-142. (Astrophysics and Space Science Library; III). https://doi.org/10.1007/978-1-4020-3407-7_24

Author

Burningham, B. ; Naylor, T. ; Littlefair, S.P. ; Jefferies, R.D. / Estimating the low-mass IMF in OB associations : o Orionis. The Initial Mass Function 50 Years Later. Springer, 2005. pp. 141-142 (Astrophysics and Space Science Library; III).

Bibtex

@inbook{347dd93ba8b141a58a568c5d0b2e70d5,
title = "Estimating the low-mass IMF in OB associations : o Orionis",
abstract = "We investigate the issues of contamination and exclusion in photometric membership selection techniques when applied to OB associations. We use radial velocities to calculate membership probabilities for a sample of very low-mass candidate members of the σ Orionis young group. We find that significant numbers of bona members are not excluded by photometric selection techniques, and for I brighter than 17 there is not significant contamination in the expected PMS region.",
author = "B. Burningham and T. Naylor and S.P. Littlefair and R.D. Jefferies",
note = "“The original publication is available at www.springerlink.com” Copyright Springer [Full text of this chapter is not available in the UHRA]",
year = "2005",
doi = "10.1007/978-1-4020-3407-7_24",
language = "English",
isbn = "978-1-4020-3406-0",
series = "Astrophysics and Space Science Library",
publisher = "Springer",
number = "III",
pages = "141--142",
booktitle = "The Initial Mass Function 50 Years Later",

}

RIS

TY - CHAP

T1 - Estimating the low-mass IMF in OB associations : o Orionis

AU - Burningham, B.

AU - Naylor, T.

AU - Littlefair, S.P.

AU - Jefferies, R.D.

N1 - “The original publication is available at www.springerlink.com” Copyright Springer [Full text of this chapter is not available in the UHRA]

PY - 2005

Y1 - 2005

N2 - We investigate the issues of contamination and exclusion in photometric membership selection techniques when applied to OB associations. We use radial velocities to calculate membership probabilities for a sample of very low-mass candidate members of the σ Orionis young group. We find that significant numbers of bona members are not excluded by photometric selection techniques, and for I brighter than 17 there is not significant contamination in the expected PMS region.

AB - We investigate the issues of contamination and exclusion in photometric membership selection techniques when applied to OB associations. We use radial velocities to calculate membership probabilities for a sample of very low-mass candidate members of the σ Orionis young group. We find that significant numbers of bona members are not excluded by photometric selection techniques, and for I brighter than 17 there is not significant contamination in the expected PMS region.

U2 - 10.1007/978-1-4020-3407-7_24

DO - 10.1007/978-1-4020-3407-7_24

M3 - Chapter

SN - 978-1-4020-3406-0

SN - 978-1-4020-3407-7

T3 - Astrophysics and Space Science Library

SP - 141

EP - 142

BT - The Initial Mass Function 50 Years Later

PB - Springer

ER -