INVESTIGATION OF LIGHT-EMISSION FROM A PARALLEL-PLATE AVALANCHE CHAMBER FILLED WITH NOBLE-GASES AND WITH TEA, TMAE, AND H2O VAPORS AT ATMOSPHERIC-PRESSURE

PESKOV, VLADIMIR; CHARPAK, G; DOMINIK, W; SAULI, F

doi:10.1016/0168-9002(89)90788-2

INVESTIGATION OF LIGHT-EMISSION FROM A PARALLEL-PLATE AVALANCHE CHAMBER FILLED WITH NOBLE-GASES AND WITH TEA, TMAE, AND H2O VAPORS AT ATMOSPHERIC-PRESSURE

PESKOV V., CHARPAK G., DOMINIK W., SAULI F.

NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, cilt.277, sa.2-3, ss.547-556, 1989 (SCI-Expanded)

Yayın Türü: Makale / Tam Makale
Cilt numarası: 277 Sayı: 2-3
Basım Tarihi: 1989
Doi Numarası: 10.1016/0168-9002(89)90788-2
Dergi Adı: NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT
Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
Sayfa Sayıları: ss.547-556
Bursa Uludağ Üniversitesi Adresli: Hayır

Özet

Astrophysical parameters (age, reddening, distance, radius, luminosity function, mass function, total mass, relaxation time and mass segregation) have been estimated for open clusters NGC 2571, NGC 6802, Koposov 53 and Be 89 by using the Two Micron All Sky Survey (2MASS) photometry. We analyse the color-magnitude diagrams and stellar radial density profiles. We have found that NGC 2571 is the youngest one having young main sequence stars while Be 89 is the oldest cluster.