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Cited article:

UTILIZING SYNTHETIC VISIBLE 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, Richard O. Gray and Christopher J. Corbally
The Astronomical Journal 153 (1) 39 (2017)
https://doi.org/10.3847/1538-3881/153/1/39

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

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.
The Astrophysical Journal 694 (1) 165 (2009)
https://doi.org/10.1088/0004-637X/694/1/165

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)
https://doi.org/10.1086/529069

Discovery of a λ Bootis Like Abundance Pattern in the Pulsating Algol-Type System RZ Cassiopeiae

Shin-ya Narusawa, Shinobu Ozaki, Eiji Kambe and Kozo Sadakane
Publications of the Astronomical Society of Japan 58 (3) 617 (2006)
https://doi.org/10.1093/pasj/58.3.617

The interferometric diameter and internal structure of Sirius A

P. Kervella, F. Thévenin, P. Morel, P. Bordé and E. Di Folco
Astronomy & Astrophysics 408 (2) 681 (2003)
https://doi.org/10.1051/0004-6361:20030994

A study of λ Bootis type stars in the wavelength region beyond 7000 Å

E. Paunzen, I. Kamp, W. W. Weiss and H. Wiesemeyer
Astronomy & Astrophysics 404 (2) 579 (2003)
https://doi.org/10.1051/0004-6361:20030284