Main sequence variables by Breger M.

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A Main Sequence for Quasars by Paola Marziani, Deborah Dultzin, Jack W. Sulentic, Ascensión Del Olmo, C. A. Negrete, Mary L. Martínez-Aldama, Mauro D'Onofrio, Edi Bon, Natasa Bon, Giovanna M. Stirpe

“…We also briefly discuss quasars in a segment of the main sequence that includes the strongest FeII emitters. …”
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THE STARS OF THE LOWER PART OF MAIN SEQUENCE by T. V. Mishenina, S. I. Belik, I. A. Usenko, O. Bienayme, C. Soubiran, V. V. Kovtyukh, S. A. Korotin

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Entropy Production of Main-Sequence Stars by Leonid M. Martyushev, Sergey N. Zubarev

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Evolution of Stars toward the Main Sequence by B. Hidajat

“…A review on the knowledge of the stellar evolution toward the main sequence is presented. This is the period during which the stars evolve from the beginning of their formation to the phase of stabilization on the main sequence where nuclear reactions begin to provide the entire energy supply.  …”
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The Pre-main Sequence: Challenges and Prospects for Asteroseismology by Konstanze Zwintz, Thomas Steindl

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An inverse-linear logistic model of the main sequence by Andrew Duchowski, Krzysztof Krejtz, Cezary Biele, Anna Niedzielska, Peter Kiefer, Ioannis Giannopoulos, Nina Gehrer, Michael Schönenberg

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Structure and Evolution of Pre-Main Sequence Stars by Schulz, Norbert S., Allen, Glenn E., Bautz, Mark W., Canizares, Claude R., Davis, John E., Dewey, Dan, Huenemoerder, David P., Heilmann, Ralf K., Houck, John C., Marshall, Herman Lee, Nowak, Michael A., Schattenburg, Mark

“…Low-mass pre-main sequence (PMS) stars are strong and variable X-ray emitters, as has been well established by EINSTEIN and ROSAT observatories. …”
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The kinematics of main-sequence stars from Hipparcos data by Binney, J, Dehnen, W, Houk, N, Murray, C, Penston, M

The properties of main-sequence stars from Hipparcos data by Houk, N, Swift, C, Murray, C, Penston, M, Binney, J

“…From this subsample we can determine the distribution in M-V of main-sequence stars of given spectral type for spectral types that range from early F to early K. …”

Hydrodynamics and Survivability during Post-main-sequence Planetary Engulfment by Ricardo Yarza, Naela B. Razo-López, Ariadna Murguia-Berthier, Rosa Wallace Everson, Andrea Antoni, Morgan MacLeod, Melinda Soares-Furtado, Dongwook Lee, Enrico Ramirez-Ruiz

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Opacity Effects on Pulsations of Main-Sequence A-Type Stars by Joyce A. Guzik, Christopher J. Fontes, Chris Fryer

“…Here we explore effects of opacity enhancements for the somewhat cooler main-sequence A-type stars, in which p-mode pulsations are driven instead in the second helium ionization region at ∼50,000 K. …”
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Mapping the Galactic halo with main-sequence and RR Lyrae stars by Sesar B.

“…We present an analysis of Galactic halo structure, substructure, and metallicity traced by main-sequence and RR Lyrae stars selected from the SDSS stripe 82 and CFHT Legacy Survey data sets. …”
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Summarized effective temperatures scale of main sequence stars and substars by M. A. Babenko, V. A. Zakhozhay

“…The generalized scale of effective temperatures (T_eff) for substars and main sequence stars in the interval spectral types Sp = O8V ÷ T9,5V. …”
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Constraining Stellar Rotation at the Zero-age Main Sequence with TESS by S. T. Douglas, P. A. Cargile, S. P. Matt, A. A. Breimann, J. A. Pérez Chávez, C. X. Huang, N. J. Wright, G. Zhou

“…The zero-age main sequence (ZAMS) is a critical phase for stellar angular momentum evolution, as stars transition from contraction-dominated spin-up to magnetic wind-dominated spin-down. …”
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The potential of space observations for pulsating pre-main sequence stars by Zwintz Konstanze

“…The first asteroseismic studies of pre-main sequence (pre-MS) pulsators have been conducted based on data from the space telescopes MOST and CoRoT with typical time bases of less than 40 days. …”
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Orbital decay in binaries containing post-main-sequence stars by Sun, M, Arras, P, Weinberg, NN, Troup, NW, Majewski, SR

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THE CHROMOSPHERES AND CORONAE OF 5 G-K MAIN-SEQUENCE STARS by Jordan, C, Ayres, T, Brown, A, Linsky, J, Simon, T

Evidence of magnetic field decay in massive main-sequence stars by Fossati, L, Schneider, F, Castro, N, Langer, N, Simón-Díaz, S, Müller, A, de Koter, A, Morel, T, Petit, V, Sana, H, Wade, G

“…A significant fraction of massive main-sequence stars show strong, large-scale magnetic fields. …”

GOODS-Herschel: an infrared main sequence for star-forming galaxies by Elbaz, D, Dickinson, M, Hwang, H, Diaz-Santos, T, Magdis, G, Magnelli, B, Le Borgne, D, Galliano, F, Pannella, M, Chanial, P, Armus, L, Charmandaris, V, Daddi, E, Aussel, H, Popesso, P, Kartaltepe, J, Altieri, B, Valtchanov, I, Coia, D, Dannerbauer, H, Dasyra, K, Leiton, R, Mazzarella, J, Alexander, D, Buat, V