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・ Pulse-address multiple access
・ Pulse-amplitude modulation
・ Pulse-chase analysis
・ Pulse-code modulation
・ Pulse-coupled networks
・ Pulse-density modulation
・ Pulse-Doppler radar
・ Pulse-Doppler signal processing
・ Pulse-Eight
・ Pulse-frequency modulation
・ Pulse-per-second signal
・ Pulse-position modulation
・ Pulse-swallowing counter
・ Pulse-width modulation
・ PulseAudio
Pulsed Accretion
・ Pulsed columns
・ Pulsed DC
・ Pulsed discharge ionization detector
・ Pulsed electromagnetic field therapy
・ Pulsed electron paramagnetic resonance
・ Pulsed energy projectile
・ Pulsed energy weapon
・ Pulsed field gradient
・ Pulsed field magnet
・ Pulsed gas dynamic spray process
・ Pulsed inductive thruster
・ Pulsed laser deposition
・ Pulsed plasma thruster
・ Pulsed power


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Pulsed Accretion : ウィキペディア英語版
Pulsed Accretion

Pulsed Accretion in astronomy is the periodic modulation in accretion rate of young stellar objects in binary systems, producing a periodic pulse in the observed infrared light curves of T Tauri stars.
In double stars in young stellar objects, a protoplanetary disk is formed around each star, accreted from matter close to the star. In such a binary star system a strongly eccentric orbit produces strong gravitational forces on the circumstellar disks at periastron, and such disturbance can lead to a temporary increase in the accretion rate onto the star. This increased accretion rate leads to a change of intensity in the infrared, such intensity rising by up to tenfold in the protostar LRLL 54361. Brightness changes in the light curve that have the same period as the orbital period of the binary system, are always assumed to be due to pulsed accretion.
==References==


抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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