Showing posts with label birth. Show all posts
Showing posts with label birth. Show all posts
Saturday, 19 August 2017
Inside Before Birth apk obb
Inside Before Birth apk obb
Jika player bangun sendirian di kegelapan dan terjebak . . .
Apa yang akan player lakukan? Melarikan diri atau melanjutkannya?
Game ini hanya mengingatkan jika . . . Ketika kegelapan memburumu, kamu tidak akan tahu apa yang nyata . . .
Cerita
Seorang gadis muda yang bernama Lucy sedang berangkat sekolah seperti hari-hari biasanya, Ketika dia sedang melihat pemandangan, dia merasakan sangat kesakitan di dalam dadanya . . . Lalu jatuh pingsan.
Dia terbangun ketika sebuah cahaya merah menyilaukan tepat mengenai wajahnya. Dia tidak sedang berada di sekolahnya . . . Terkunci di sebuah ruangan . . . Dia terbangun di sebuah ruangan yang berwarna merah.
Bisakah anda seorang player atau gamer membantunya?
Fitur
- Puzzle yang rumit, player perlu menjelajah dan menggunakan logika untuk menyelesaikannya.
- Menyeramkan <- sudah pasti.
- Story di sampaikan dengan visual.
- Grafis full 3D.
- Game di optimalkan dengan tingkat grafis yang berbeda dan kontrol kecerahan.
- Suara 3D
TESTING Samsung Galaxy J5 Lollipop
MODE Offline
REQUIRED: Android OS 4.0 And Up
"Grafis full 3D"
"Player akan berperan sebagai lucy"
"Cerita yang penuh misteri"
Inside Before Birth v4.1
Inside Before Birth v4.1
apk -> download <- 34.3mb
obb -> download <- 203.6mb
Petunjuk...!!!
- Download
- Extrak file "zip" nya dengan winrar/zip (kalo tidak punya pc, teman-teman bisa memakai aplikasi android dengan memasangnya dari >>> Play Store <<< atau instal file apknya dengan >>> Unrar Pro <<< )
- Instal gamenya (cukup klik file "apk" di file manager.)
- Taruh data di Sdcard/android/obb/di sini guys (kalau belum ada "BUAT" foldernya manual)
- Selamat memainkan gamenya guys......
Akhir kata, terima kasih telah mengunjungi Blog saya yang masih cupu ini.... hehehe
download file now
Friday, 18 August 2017
Perseus Cluster and Virgo Cluster NASAs Chandra Observatory Identifies Impact of Cosmic Chaos on Star Birth
Perseus Cluster and Virgo Cluster NASAs Chandra Observatory Identifies Impact of Cosmic Chaos on Star Birth
- Chandra observations of two galaxy clusters suggest turbulence may be preventing hot gas there from cooling.
- This addresses a long-standing question of why the vast amounts of hot gas in clusters do not cool to form large numbers of stars.
- Previous work showed supermassive black holes at the centers of the clusters play a key role in this process.
- The new finding about turbulence helps fill a gap in the understanding of these giant clusters of galaxies.
These two Chandra images of galaxy clusters - known as Perseus and Virgo - have provided direct evidence that turbulence is helping to prevent stars from forming. These new results could answer a long-standing question about how these galaxy clusters keep their enormous reservoirs of hot gas from cooling down to form stars.
Galaxy clusters are the largest objects in the Universe held together by gravity. They contain hundreds or thousands of individual galaxies that are immersed in gas with temperatures of millions of degrees. This hot gas, which is the heftiest component of the galaxy clusters aside from dark matter, glows brightly in X-ray light. Over time in the centers of clusters, this gas should cool enough so that stars form at prodigious rates. This, however, is not what astronomers have observed in many galaxy clusters.
A team of researchers have found evidence that the heat is generated by turbulent motions, which they identified from signatures in the Chandra data. Previously, other scientists have shown the key role of supermassive black holes in the centers of large galaxies in the middle of galaxy clusters. These black holes pump vast quantities of energy into the volumes around them through powerful jets of energetic particles. Chandra and other X-ray telescopes have detected giant cavities created in the hot cluster gas by the jets.
The latest research provides insight into just how energy can be transferred from the cavities to the surrounding gas. The interaction of the cavities with the gas may be generating turbulence, or chaotic motion similar to that on a bumpy airplane ride, which then dissipates to keep the gas hot for billions of years.
The scientists targeted Perseus and Virgo because they are both extremely large and relatively bright, thus providing an opportunity to see details that would be very difficult to detect in other clusters. The evidence for turbulence can be seen most clearly in the ripple-like structures in the Chandra image of Perseus. When combined with careful analysis of the data with theoretical models, this new result provides the clearest evidence to date that turbulence is the mechanism that prevents the hot gas in these clusters from cooling.
Image Credit: NASA/CXC/Stanford/I.Zhuravleva et al
Explanation from: http://chandra.harvard.edu/photo/2014/perseusvirgo/
download file now
Friday, 11 August 2017
Subscribe to:
Posts (Atom)