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Cited article:

Identification of emission-line stars in transition phase from pre-main sequence to main sequence

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Interstellar Extinction in the Direction of the Young Open Cluster NGC 6530

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Publications of the Astronomical Society of the Pacific 132 (1010) 044301 (2020)
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Orbit and physical characteristics of the components of the massive Algol V622 Per, a member of the open star cluster χ Per

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Astronomy Letters 42 (10) 674 (2016)
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Profiles of the Hα and Hβ lines in the spectra of B and Be stars in the diffuse stellar cluster h/χ Persei

S. L. Malchenko and A. E. Tarasov
Astrophysics 51 (2) 250 (2008)
https://doi.org/10.1007/s10511-008-9002-z

XMM-Newton observation of the Be/neutron star system RX J0146.9+6121: a soft X-ray excess in a low luminosity accreting pulsar

N. La Palombara and S. Mereghetti
Astronomy & Astrophysics 455 (1) 283 (2006)
https://doi.org/10.1051/0004-6361:20065107

H [CSC]ii[/CSC] Emission from a Complete Spectroscopic Survey of B[CLC]e[/CLC] Stars in [CLC]h[/CLC] and χ Persei

Ann E. Bragg and Scott J. Kenyon
The Astronomical Journal 124 (6) 3289 (2002)
https://doi.org/10.1086/344306

[ITAL]UBVI[/ITAL] and Hα Photometry of the [CLC][ITAL]h[/ITAL][/CLC] and χ Persei Cluster

Stefan C. Keller, Eva K. Grebel, Grant J. Miller and Kenneth M. Yoss
The Astronomical Journal 122 (1) 248 (2001)
https://doi.org/10.1086/321139