70 research outputs found
Measuring-analytical complex for investigation of local C-V- characteristics of semiconductor barrier structures on the basis of AFM
Π Π°Π·ΡΠ°Π±ΠΎΡΠ°Π½ Π°Π²ΡΠΎΠΌΠ°ΡΠΈΠ·ΠΈΡΠΎΠ²Π°Π½Π½ΡΠΉ ΠΈΠ·ΠΌΠ΅ΡΠΈΡΠ΅Π»ΡΠ½ΡΠΉ ΠΊΠΎΠΌΠΏΠ»Π΅ΠΊΡ Π΄Π»Ρ Π»ΠΎΠΊΠ°Π»ΡΠ½ΠΎΠ³ΠΎ ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΡ Π²ΠΎΠ»ΡΡ-ΡΠ°ΡΠ°Π΄Π½ΡΡ
Ρ
Π°ΡΠ°ΠΊΡΠ΅ΡΠΈΡΡΠΈΠΊ ΠΏΠΎΠ»ΡΠΏΡΠΎΠ²ΠΎΠ΄Π½ΠΈΠΊΠΎΠ²ΡΡ
ΡΡΡΡΠΊΡΡΡ Π½Π° ΠΎΡΠ½ΠΎΠ²Π΅ Π·ΠΎΠ½Π΄ΠΎΠ²ΠΎΠΉ ΡΠΈΡΡΠ΅ΠΌΡ Π°ΡΠΎΠΌΠ½ΠΎ-ΡΠΈΠ»ΠΎΠ²ΠΎΠ³ΠΎ ΠΌΠΈΠΊΡΠΎΡΠΊΠΎΠΏΠ°.Automated measuring complex for local research of capacitor-voltage characteristics of semiconductor structures based on the probe system of an atomic force microscope has been developed.Π Π°Π±ΠΎΡΠ° Π²ΡΠΏΠΎΠ»Π½Π΅Π½Π° ΠΏΡΠΈ ΡΠΈΠ½Π°Π½ΡΠΎΠ²ΠΎΠΉ ΠΏΠΎΠ΄Π΄Π΅ΡΠΆΠΊΠ΅ Π Π€Π€Π (Π³ΡΠ°Π½Ρ 16-32-00342) Ρ ΠΈΡΠΏΠΎΠ»ΡΠ·ΠΎΠ²Π°Π½ΠΈΠ΅ΠΌ ΠΎΠ±ΠΎΡΡΠ΄ΠΎΠ²Π°Π½ΠΈΡ Π Π΅Π³ΠΈΠΎΠ½Π°Π»ΡΠ½ΠΎΠ³ΠΎ ΡΠ΅Π½ΡΡΠ° Π·ΠΎΠ½Π΄ΠΎΠ²ΠΎΠΉ ΠΌΠΈΠΊΡΠΎΡΠΊΠΎΠΏΠΈΠΈ ΠΊΠΎΠ»Π»Π΅ΠΊΡΠΈΠ²Π½ΠΎΠ³ΠΎ ΠΏΠΎΠ»ΡΠ·ΠΎΠ²Π°Π½ΠΈΡ (Π Π¦ΠΠΠΊΠΏ) ΠΏΡΠΈ Π€ΠΠΠΠ£ ΠΠ Β«Π ΠΠ Π’Π£Β» (ckp.rsreu.ru) Π² ΠΠΠ¦ Π½Π΅ΡΠΏΠΎΡΡΠ΄ΠΎΡΠ΅Π½Π½ΡΡ
ΠΈ Π½Π°Π½ΠΎΡΡΡΡΠΊΡΡΡΠΈΡΠΎΠ²Π°Π½Π½ΡΡ
ΠΌΠ°ΡΠ΅ΡΠΈΠ°Π»ΠΎΠ² ΠΈ ΡΡΡΡΠΎΠΉΡΡΠ² Π½Π° ΠΈΡ
ΠΎΡΠ½ΠΎΠ²Π΅ (ΠΠΠΠ£)
Spectroscopy and Photometry of MWC 137
MWC 137 is an object with a strong emission-line spectrum associated with an 1'-size H Imall> region Sharpless 266. It was included in a catalog of planetary nebulae in 1967, in the first list of objects with the B[e] phenomenon in 1976, and in a list of Herbig Ae/Be stars in 1984. A recent analysis of the stellar and nebular spectra of MWC 137 by several authors suggested that it is most likely a B[e] supergiant located at a distance 4-6 kpc away from the Sun. No high-resolution spectra of the object have been published so far. We present the results of our analysis of high-resolution optical spectra of MWC 137 obtained in 2004-2016 and UBVRI photometry
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