Size: 332.87 MB | Total Duration: 02:23:22 | Total Tracks: 40
Format: MPEG Audio | 320 Kbps
Album: Active Spring
Artist: VA
Genre: Dance
Date/Year: 2022

Total tracks: 40 | Size: 332.87 MB | Formats: mp3

Total tracks: 40 | Size: 314.38 MB | Formats: mp3

MP4 | Video: h264, 1280x720 | Audio: AAC, 44.1 KHz, 2 Ch
Genre: eLearning | Language: English + srt | Duration: 23 lectures (4h 23m) | Size: 2 GB
How to automate active directory based demo labs for pentesting, hacking and training requirements

Russian Active Measures Yesterday, Today, Tomorrow by Olga Bertelsen PDF | 3.88 MB
N/A | 419 Pages

Title: N/A
Author: N/A
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LinkedIn Learning
Duration: 1h 28m | .MP4 1280x720, 30 fps(r) | AAC, 48000 Hz, 2ch | 779 MB
Genre: eLearning | Language: English

Active Side Of Infinity The Carlos Castaneda
epub | 255.21 KB | English | Isbn:‎ 978-0060929602 | Author: Carlos Castaneda | Year: 1999

English | 2020 | ISBN: 0750332778 | 382 pages | True (PDF,EPUB,MOB) | 120.44 MB
This book looks at analysis and modelling of active biopotential signal processing. It emphasises the real-time challenges in

English | 2021 | ISBN: 0750330333 , 978-0-7503-3035-0 | 116 pages | True PDF EPUB MOBI | 64.77 MB
Almost all galaxies host in their center a supermassive black hole of mass between a million and tens of billions solar masses. Supermassive black holes grow in symbiosis with their host galaxies across the Hubble time, occasionally accreting surround matter, giving rise to an Active Galactic Nuclei (AGN). This book gives a general review of our current knowledge of AGN, powered by supermassive black holes: how they are fueled by gas (or stars) and what problems are encountered; how can we account for the wide variety of AGN, from Seyfert/Liners to quasars, and for the two types (AGN 1 and 2) either through dust obscuration, and geometrical orientation arguments, or through intrinsic activity difference, qualitative or quantitative. With modern instruments, providing high resolution and sensitivity, like ALMA in radio, or MUSE at the ESO/VLT, it is possible to unveil the interstellar medium and stars in the circumnuclear regions, discover molecular disks and tori, in the sphere of influence of the black holes. While AGN are accreting matter, they are providing so much energy that part of the surrounding gas is expelled and is observed in molecular outflows, identified as the main feedback process of AGN on their host.

Thinking Like an Engineer An Active Learning Approach by Elizabeth A Stephan PDF | 12.4 MB
N/A | 799 Pages

Title: 0133595412.pdf
Author: N/A
Year: N/A