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Vasubandhu: Abhidharmakośabhāṣya

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ā ī ū
ñ
ś ź
š č ǰ γ    
Note on the transliteration:
The transliteration system of the BP/TLB is based on the Unicode/UTF-8 system. However, there may be difficulties with some of the letters – particularly on PC/Windows-based systems, but not so much on the Mac. We have chosen the most accepted older and traditional systems of transliteration against, e.g, Wylie for Tibetan, since with Unicode it is possible, in Sanskrit and Tibetan, etc., to represent one sound with one letter in almost all the cases (excepting Sanskrit and Tibetan aspirated letters, and Tibetan tsa, tsha, dza). We thus do not use the Wylie system which widely employs two letters for one sound (ng, ny, sh, zh etc.).
 
Important:
We ask you in particular to note the use of the ’ apostrophe and not the ' representing the avagrāha in Sanskrit, and most important the ’a-chuṅ in Tibetan. On the Mac the ’ is Alt-M.
 
If you cannot find the letters on your key-board, you may click on the link "Diacritica" to access it for your search.
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Click to Expand/Collapse OptionTitle
Click to Expand/Collapse OptionPreface
Click to Expand/Collapse OptionChapter I: Dhātunirdeśa
Click to Expand/Collapse OptionChapter II: Indriyanirdeśa
Click to Expand/Collapse OptionChapter III: Lokanirdeśa
Click to Expand/Collapse OptionChapter IV: Karmanirdeśa
Click to Expand/Collapse OptionChapter V: Anuśayanirdeśa
Click to Expand/Collapse OptionChapter VI: Mārgapudgalanirdeśa
Click to Expand/Collapse OptionChapter VII: Jñānanirdeśa
Click to Expand/Collapse OptionChapter VIII: Samāpattinirdeśa
Click to Expand/Collapse OptionChapter IX: Conclusions
San: Pradhan (1967) 124,7-124,8
ata eva yamalayoryaḥ paścāt prajāyate sa jyāyānucyate yaḥ pūrvaṃ sa kanīyāniti |
Chi: 真諦 Zhēndì 563-568 A.D. T.1559 202c10-11
是故雙生。若在後(11)生爲大。若在前生爲小。
Chi: 玄奘 Xuánzàng 651 A.D. T 1558 46a2
故雙生者前小後大。
Tib: Jinamitra/dPal brtsegs, ca. A.D. 800, Tg, mṅon pa, ku
de ñid kyi phyir mtshe ma las gaṅ phyis byuṅ ba de ni nu bo źes bya’o || gaṅ sṅar byuṅ ba de ni phu bo źes bya’o ||
Nor
.
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