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Cited article:

Discovery of λ Boo stars in open clusters

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UTILIZING SYNTHETIC VISIBLE SPECTRA TO EXPLORE THE PHYSICAL BASIS FOR THE CLASSIFICATION OF LAMBDA BOÖTIS STARS

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The Astronomical Journal 153 (1) 39 (2017)
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The Discovery of λ Bootis Stars: The Southern Survey I

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UTILIZING SYNTHETIC UV SPECTRA TO EXPLORE THE PHYSICAL BASIS FOR THE CLASSIFICATION OF LAMBDA BOÖTIS STARS

Kwang-Ping Cheng, James E. Neff, Dustin M. Johnson, Erik S. Tarbell, Christopher A. Romo, Arvind Prabhaker, Patricia A. Steele, Richard O. Gray and Christopher J. Corbally
The Astronomical Journal 151 (4) 105 (2016)
https://doi.org/10.3847/0004-6256/151/4/105

IR excesses around nearby Lambda Boo stars are caused by debris discs rather than ISM bow waves

Z. H. Draper, B. C. Matthews, G. M. Kennedy, et al.
Monthly Notices of the Royal Astronomical Society 456 (1) 459 (2016)
https://doi.org/10.1093/mnras/stv2696

An Evaluation of the Membership Probability of 212 λ Boo Stars. I. A Catalogue

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Publications of the Astronomical Society of Australia 32 (2015)
https://doi.org/10.1017/pasa.2015.34

λ Bootis stars in the SuperWASP survey

E. Paunzen, M. Skarka, P. Walczak, et al.
Monthly Notices of the Royal Astronomical Society 453 (2) 1241 (2015)
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Investigating the possible connection betweenλBootis stars and intermediate Population II type stars

E. Paunzen, I. Kh. Iliev, L. Fossati, U. Heiter and W. W. Weiss
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SPECTRAL IRRADIANCE CALIBRATION IN THE INFRARED. XVII. ZERO-MAGNITUDE BROADBAND FLUX REFERENCE FOR VISIBLE-TO-INFRARED PHOTOMETRY

Charles W. Engelke, Stephan D. Price and Kathleen E. Kraemer
The Astronomical Journal 140 (6) 1919 (2010)
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INFRARED EMISSION BY DUST AROUND λ BOOTIS STARS: DEBRIS DISKS OR THERMALLY EMITTING NEBULAE?

J. R. Martínez-Galarza, I. Kamp, K. Y. L. Su, et al.
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Could the Ultra–Metal‐Poor Stars be Chemically Peculiar and Not Related to the First Stars?

K. A. Venn and David L. Lambert
The Astrophysical Journal 677 (1) 572 (2008)
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Modeling the Infrared Bow Shock at δ Velorum: Implications for Studies of Debris Disks and λ Bootis Stars

A. Gaspar, K. Y. L. Su, G. H. Rieke, et al.
The Astrophysical Journal 672 (2) 974 (2008)
https://doi.org/10.1086/523299