Pik Sin The
Bosscha Observatory, Lembang (Java)

Published : 3 Documents Claim Missing Document
Claim Missing Document
Check
Articles

Found 3 Documents
Search

Identification Charts for Planetary Nebulae Pik Sin The
Journal of Mathematical and Fundamental Sciences Vol. 3 No. 2 (1964)
Publisher : Institute for Research and Community Services (LPPM) ITB

Show Abstract | Download Original | Original Source | Check in Google Scholar

Abstract

Abstract. At Dr. L. Perek's request, identification charts for 12 known planetary nebulae, of which the locations were not certain, are given. Ichtisar. Atas permintaan Dr. L. Perek, peta pengenal untuk 12 kabut planit jang letaknja diragukan, disadjikan dalam tulisan ini.
New H-ALPHA Emission Stars in A Region to the East of the T-Association Near Rho Ophiuci Pik Sin The; Ham Keng Lim
Journal of Mathematical and Fundamental Sciences Vol. 3 No. 1 (1964)
Publisher : Institute for Research and Community Services (LPPM) ITB

Show Abstract | Download Original | Original Source | Check in Google Scholar

Abstract

The result of a survey of H-alpha emission objects in an area of approximately 25 square degrees centered on the star CD -24°12765 (R.A.=16h38.m5; Dec.=-24°22';1950), is presented. Only 33% of H-alpha emission stars discovered by Dolidze and Arakelyan (1959) which are located in  the present survey region, are redetected in our plates. A total number of 32 new H-alpha emission objects are found. Their position and finding charts are given.
Faint Hα-Emission Objects in Nebulosities Surrounding the Star m Cen. Pik Sin The
Journal of Mathematical and Fundamental Sciences Vol. 2 No. 1 (1962)
Publisher : Institute for Research and Community Services (LPPM) ITB

Show Abstract | Download Original | Original Source | Check in Google Scholar

Abstract

Tudjuh puluh delapan buah bintang Hα-emisi jang baru dan dua buah kabut-planit telah diketemukan pada suatu survey dalam daerah kabut gelap dan bertjahaja pada lingkungan bintang m Cen. Pusat daerah ini terletak pada Î±=13h04m; δ=-63°30'(1875). Posisi kira-kira magnitudo V dan warna V-R telah ditentukan. Peta-peta jang menundjukkan letak benda-benda itu dilampirkan.Di antara bintang-bintang emisi ternjata ada 12 buah jang mungkin merupakan bintang berubah. Hal ini menjokong kesimpulan bahwa sebagian daripada bintang emisi jang lemah tjahajanya mungkin membentuk asosiasi-asosiasi T jang mempunjai hubungan dengan kabut-kabut  tersebut di atas dan mungkin djuga mempunyai hubungan dengan asosiasi OB jang dinamakan I-Cru.