RT And * CB EA RS 8.97 0.41 0.31 V 0.6289 v 170 000 170 000 F8V+K1 a 231110.1 +530133 SY And SA * EA 10.70 1.50 V 34.9085 060 027 A0+K1 001316.4 +434241 TT And * SA EA 11.50 1.50 0.10 V 2.7651 v 140 000 A+G7IV 231322.9 +460851 TW And * SA EA 8.98 2.06 0.15 V 4.1228 v 130 020 F0V+K0 000318.2 +325045 UU And SA EA 11.20 3.00 0.20 V 1.4863 v 170 000 A8IV/V 004345.1 +305620 WW And * SA EA 10.92 0.67 0.16 V 23.2852 050 000 000 A0:+G5-K0III 234453.5 +454112 WX And SA * EA 12.10 1.70 V 3.0011 d 120 030 F5IV
... DII, without confirmation CD And System can belong to DGlate only because of its large period, but A2 is not suitable for DG. ... Only old photographic data are available. ... V395 And C May belong to CE only but spectra is somewhat later than needed V413 And Period is large to classify as SA, period is short to classify as DGlate. ... V1464 Aql C ELL+DSCT in VSX, RR in Simbad, confirmation is needed ER Ara Value of A2 is large, old photographic data only. ... Only old photographic data are known. ...
RT And ChromActive 125 RT And PeriodVar 215 TT And SpType 213 TT And PeriodVar 213 TW And PeriodVar 213 WW And SpType 140 WW And dII 140 WW And dI 140 XZ And SpType 213 XZ And PeriodVar 213 AB And PeriodVar 213 BD And SystemClass 173 BX And PeriodVar 215 CD And Period 1 CN And PeriodVar 352 CU And Period 1 EL And Max 124 EL And A1 124 EL And A2 ...
FF Aqr DW Period is significantly greater than typical value for DW type. According to Pojmanski [45] this star is DCEP-FU: variable. According to Sipahi et al. [263] it is one of the few binary systems which consists of the hot subdwarf and cool chromospherically active giant components. ... Belongs to long-period RS CVn systems, secondary is more massive and more larger (volume of the secondary is approximately 100 times larger than that of the primary component). ... So may be SA system? ...
Olga V. Kochina . ... Russia, Moscow, 119017, . ... Modeling the synthesis of complex molecules in protostellar objects', Kochina O. V., Wiebe D. S., Vasyunin A. I., 2012, Physics of the Universe, Conference for young scientists, Ekaterinburg, Russia . Modeling of the formation of complex molecules in protostellar objects', Kochina O. V., Wiebe D. S., Kalenskii S.V., Vasyunin A. I.,2013 Astronomy Reports, Vol. 57(11), pp: 818 - 832 . ... Ultraviolet Universe - 2010", Saint-Petersburg, Russia. ...
zet And ELL+RS 431 NW Aur CST 99 FH Cam DSCT 428 EF Cnc RRC 93 VW CVn RRC 94 CU CVn DSCT 428 TZ Cap RRAB 20 GG Car BE+R: 426 V445 Cen CWA 45 VW Cet CST 87 CI Com RRC: 91 V939 Cyg RRC 92 V1507 Cyg notE 438 gam Dor GDOR 96 BM Eri SR 53 AW Gru SR 427 TY Leo CST 98 FO Leo SR 429 RY Lep DSCT 48 V480 Lyr RVA 17 V559 Lyr L 430 V769 Mon GDOR 97 V378 Oph RVA 19 V945 Oph RRAB 91 V1366 Ori UXOR+DSCT 53 V410 Peg CST 196 V718 Per notE 437 XY Pic DSCT 418 RU Sex RRAB 425 FX Vel UXOR 53
CN And CWA_CB According to lc from Jassur & Khodadadi [352] it is a CBV system because of asymmetry (primary maximum is greater than secondary) and large dA, but according to lc solution it is CWA overcontact system with components in poor termal contact. ... According to Coughlin et al. [354] is a marginal contact system with both components almost fill their critical lobes, light curve asymmetric, so authors use hot spot on the primary to solve light curves. ... So It may be the CW system. ...
. Dluzhnevskaya Olga B. - head of the group . Piskunov Anatolij E. Vereshchagin Sergey V. Chupina Natalia V. Kovaleva Dana A. Please send your questions and comments to www.inasan.rssi.ru .
RUSSIAN . The Centre for Astronomical Data (CAD) of the Institute of Astronomy (INASAN) of the Russian Academy of Sciences was established in 1980 as a branch regional center of the Centre de Donnes Stellaire (CDS) with the purpose of astronomical data dissemination among Soviet and Eastern Europe astronomers and for providing the CDS with Soviet machine readable astronomical catalogues. The CAD archive is based on astronomical catalogues received from Strasbourg since 1980. ...
... Центр астрономических данных (ЦАД) Института астрономии (ИНАСАН) Российской академии наук был образован в 1980 году как филиал Страсбургского центра данных ( Centre de Donnes Stellaire (CDS) с целью распространения астрономических данных среди астрономов СССР и стран Восточной Европы, а также для пополнения CDS машиночитаемыми версиями астрономических каталогов, создаваемых в СССР. Основу архива ЦАД составляют астрономические каталоги, регулярно получаемые из Страсбурга с 1980 года. ...
. ENGLISH . Длужневская О.Б. - руководитель . Пискунов А.Э. Верещагин С.В. Ковалева Д.А. Чупина Н.В. Please send your questions and comments to www.inasan.rssi.ru
RUSSIAN . Full name: . Institute of Astronomy of the Russian Academy of Sciences . ... INASAN . Name before 1990: . Astronomical Council of the Academy of Sciences USSR . ... Phone : . 7 (495) 951-54-61 . ... admin@inasan.rssi.ru . ... Director: . ... Boyarchuk Alexander A. Vice Director : . Bisikalo Dmitry V. Vice Director : . ... Ptitsyn Dmitry A. Accountancy . ... Funtikova Irina V. phone: 953-29-94 . ...