Hayflick limit - ορισμός. Τι είναι το Hayflick limit
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Τι (ποιος) είναι Hayflick limit - ορισμός


Hayflick limit         
  • bases]] lie horizontally between the two spiraling strands. [[Nitrogen]]: blue, [[oxygen]]: red, [[carbon]]: green, [[hydrogen]]: white, [[phosphorus]]: orange
  • The typical normal human fetal cell will divide between 50 and 70 times before experiencing senescence. As the cell divides, the telomeres on the ends of chromosomes shorten. The Hayflick limit is the limit on cell replication imposed by the shortening of telomeres with each division. This end stage is known as [[cellular senescence]].
NUMBER OF TIMES A NORMAL HUMAN CELL POPULATION WILL DIVIDE UNTIL CELL DIVISION STOPS; (IN CULTURE) PHENOMENON, WHEN FIBROBLASTS CAN REACH A MAXIMUM OF 50 CELL DIVISIONS BEFORE BECOMING SENESCENT
Hayflick Limit; Hayflick theory; Henflick limit; Haystack limit; Replicative senescence; The hayflick limit; Hayflick number; Hayflick's limit; Hayflick phenomenon
The Hayflick limit, or Hayflick phenomenon, is the number of times a normal somatic, differentiated human cell population will divide before cell division stops. However, this limit does not apply to stem cells.
Detection limit         
FOR A GIVEN ANALYTICAL PROCEDURE, CONCENTRATION OR QUANTITY DERIVED FROM THE SMALLEST MEASURE THAT CAN BE DETECTED WITH REASONABLE CERTAINTY
Limit of detection; Limit of Detection; Detection Limits; Limit of quantification; LOQ; Limit of quantitation
The limit of detection (LOD or LoD) is the lowest signal, or the lowest corresponding quantity to be determined (or extracted) from the signal, that can be observed with a sufficient degree of confidence or statistical significance. However, the exact threshold (level of decision) used to decide when a signal significantly emerges above the continuously fluctuating background noise remains arbitrary and is a matter of policy and often of debate among scientists, statisticians and regulators depending on the stakes in different fields.
Tolman–Oppenheimer–Volkoff limit         
UPPER BOUND TO THE MASS OF COLD, NONROTATING NEUTRON STARS
TOV limit; Oppenheimer–Volkoff limit; Tolman-Oppenheimer-Volkov limit; Oppenheimer-Volkov limit; Tolman-Oppenheimer-Volkoff limit; Tolman-Oppenheimer-Volkoff Limit; Oppenheimer-Volkoff limit
The Tolman–Oppenheimer–Volkoff limit (or TOV limit) is an upper bound to the mass of cold, nonrotating neutron stars, analogous to the Chandrasekhar limit for white dwarf stars. If the mass of the said star reaches the limit it will collapse to a denser form.