Results 171 to 180 of about 11,683 (215)
Nature's economy as blueprint: regional overlap & block-based algorithm for protein design. [PDF]
Retana-Fonseca HA +3 more
europepmc +1 more source
Evaluation of non-canonical p53 functions in DNA replication and recombination for variant classification. [PDF]
Jansche R +11 more
europepmc +1 more source
A Faint Progenitor System for the Faint Supernova 2024vjm
Zimmerman E +69 more
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V3101 Cyg: A Cataclysmic Variable Born with a Brown Dwarf Donor
Ramirez S +7 more
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The ages of pre-main-sequence stars [PDF]
The position of pre-main-sequence or protostars in the Hertzsprung--Russell diagram is often used to determine their mass and age by comparison with pre-main-sequence evolution tracks. On the assumption that the stellar models are accurate, we demonstrate that, if the metallicity is known, the mass obtained is a good estimate.
Christopher A Tout +2 more
exaly +3 more sources
Timescale of mass accretion in pre-main-sequence stars [PDF]
We present initial result of a large spectroscopic survey aimed at measuring the timescale of mass accretion in young, pre-main-sequence stars in the spectral type range K0 - M5. Using multi-object spectroscopy with VIMOS at the VLT we identified the fraction of accreting stars in a number of young stellar clusters and associations of ages between 1 ...
D Fedele +2 more
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Infrared companions to pre-main sequence stars
Astrophysics and Space Science, 1988We report 1.2, 1.6, 2.2 and 3.6 μm slit scan observations of the young low-luminosity stars Elias 22 (also known as GSS 31) in the Rho Ophiuchus dark cloud and Glass I in the Chamaeleon dark cloud. We discovered an infrared companion to Elias 22 at a projected separation of 2.0 arcsec (320 AU) and an optical/infrared companion to Glass I at a projected
H. Zinnecker +4 more
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Pre-Main-Sequence Binary Stars
Annual Review of Astronomy and Astrophysics, 1994The observational study of pre-main-sequence (PMS) binary stars is in many ways a very young field; most PMS binaries known today were discovered in the past decade. Nonetheless, T Tauri stars have been under study for more than a half century, and the serendipitous discovery of visual pairs has always been a by-product of their observation (e.g. Joy &
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