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10981. Презентация PowerPoint
. Prague, August 16, 2006 . Present classification : Suggested: . CW, CWA, CWB CW (period will also be given) DSCT, DSCTC, SXPHE DSct (amplitude will also be given, population membership is not always obvious) . L, LB, LC L, Lb (for red stars) . M M . PVTEL PVTel . RR, RRAB, RRC, RR(B) RR, RR0, RR1, RRB01 . RV, RVA, RVB RV, RVb (if the secondary wave?s . amplitude is at least equal to that of . the main oscillation) . PULSATING VARIABLES (CONTINUED)
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/slide0017.htm -- 7.5 Кб -- 04.09.2006
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10982. Презентация PowerPoint
. Prague, August 16, 2006 . Present classification : Suggested: SR, SRA, SRB, SRC, SRS SR (the regularity level should be indicated by the presentation of the light elements; if a star is a supergiant, it will be obvious from its spectral type) SRD SRd (we feel not inclined to introduce the UU Her type) ZZ, ZZA, ZZB, ZZO ZZ (subtype is contained in the spectral type) . BLBOO BLBoo . GDOR GDor . PULSATING VARIABLES (CONTINUED)
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/slide0018.htm -- 7.6 Кб -- 04.09.2006
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10983. Презентация PowerPoint
. Prague, August 16, 2006 . Present classification : Suggested: RPHS RPHS (rapidly pulsating hot subdwards; we repeat our call for suggestions of a better designation) . LPB or LBV SPB . PULSATING VARIABLES (CONTINUED)
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/slide0019.htm -- 6.0 Кб -- 04.09.2006
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10984. Презентация PowerPoint
. Prague, August 16, 2006 . Present classification : Suggested: . FU, I, IA, IB, INA, INB, I, TT, TTc, TTw, HAeBe . INT, IT, IN(YY), IS, ISA, Remark: I is for irregulars with . ISB doubts about their being young, . TTc for classical and TTw, for weak-lined T Tauri stars, HAeBe for Herbig Ae/Be stars . GCAS, BE Be . RCB RCB . RS Move to rotating variables . SDOR SDor . UV, UVN UV . ERUPTIVE VARIABLES
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/slide0020.htm -- 7.6 Кб -- 04.09.2006
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10985. Презентация PowerPoint
. Prague, August 16, 2006 . Present classification : Suggested: . WR WR . ? New type: PP (a proto-planetary object) New type: dL (L dwarf), the causes of variability not quite clear yet . ERUPTIVE VARIABLES (CONTINUED)
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/slide0021.htm -- 6.6 Кб -- 04.09.2006
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10986. Презентация PowerPoint
. Prague, August 16, 2006 . Present classification : Suggested: . ACV, SXARI ACV . ACVO roAp, ACV+roAp BY BY; also should include chromospherically active giants . ELL Ell . FKCOM FKCom . PSR Psr . R R . ? RS (earlier among eruptive) . ROTATING VARIABLES
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/slide0022.htm -- 7.3 Кб -- 04.09.2006
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10987. Презентация PowerPoint
. Prague, August 16, 2006 . Present classification : Suggested: . No subtype: CV N, NA, NB N, Nhf (final helium flash; suggestions of a different designation are welcome) NR Nr, NSym (symbiotic Nova), UGWZ (see below) . NC NSym NL CV, UXUMa (?permanent outburst?), VY (VY Scl type, fadings from time to time) . CATACLYSMIC VARIABLES . AND OTHER STARS WITH OUTBURSTS
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/slide0023.htm -- 7.6 Кб -- 04.09.2006
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10988. Презентация PowerPoint
. Prague, August 16, 2006 . Present classification : Suggested: . SN, SNI, SNII SN (to avoid introducing the current complex classification) AM AM (including XM from X-ray variables), DQ (intermediate polars) . UG, UGSS, UGZ UG, UGSS, UGZ UGSU UGSU, UGWZ (WZ Sge type, extremely long supercycles, large amplitudes), UG_ER (ER Uma type, short supercycles and normal cycles, small amplitudes; ideas of a better abbreviation are welcome) . CATACLYSMIC VARIABLES . AND OTHER STARS WITH OUTBURSTS (CONTINUED)
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/slide0024.htm -- 7.8 Кб -- 04.09.2006
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10989. Презентация PowerPoint
. Prague, August 16, 2006 . Present classification : Suggested: . ZAND Sym, NSym . CATACLYSMIC VARIABLES . AND OTHER STARS WITH OUTBURSTS (CONTINUED)
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/slide0025.htm -- 5.4 Кб -- 04.09.2006
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10990. Презентация PowerPoint
. Prague, August 16, 2006 . Present classification : Suggested: . E, EA, EB, EW, EP E, EA, EC ? contact (merging EB and EW), EP PN, WD, WR Remove from the classification, indicate through the spectral type or Remarks RS If such a star has eclipses, give notation like EA+RS, RS+EA . AR, D, DM, DS, DW, K, Remove from the classification; KE, KW, SD as a rule, these types in the GCVS are based on indirect evidence . ECLIPSING VARIABLES . (the description of the class should not mention close binarity)
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/slide0026.htm -- 7.8 Кб -- 04.09.2006
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10991. Презентация PowerPoint
. Prague, August 16, 2006 . Present classification : Suggested: . X, XB, XF, XI, XJ, XND, AM (move to cataclysmics), X, X N, XNB (approximately corresponds to XNG, a B star orbiting a compact object), Xlm (low mass), Xhm (high mass), Xmq (microquasars). In this class, advice from experts is especially needed . X-RAY VARIABLES
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/slide0027.htm -- 7.0 Кб -- 04.09.2006
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10992. Презентация PowerPoint
Prague, August 16, 2006 . ... Continue the GCVS project for at least 3 ?6 more years; • ? for this period, continue publication of Name-Lists for individual discoveries and for large-survey stars studied also elsewhere; • ? during this period, start a new GCVS version with improved data and with complete information for Name-List stars; . during this period, work on Steve Kawaler?s suggestion; • ? pay maximum attention to improving software for period determination, automatic classification, etc . ...
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/slide0033.htm -- 7.2 Кб -- 04.09.2006
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10993. Презентация PowerPoint
. Данная презентация содержит объекты, не отображаемые используемым обозревателем. Она рассчитана на просмотр с помощью более поздних версий Microsoft Internet Explorer. Если вы все же хотите продолжить, щелкните здесь .
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.htm -- 3.5 Кб -- 04.09.2006
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10994. Презентация PowerPoint
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Ссылки http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/frame.htm -- 2.3 Кб -- 04.09.2006
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10995. http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/master01.htm
. 'верхний колонтитул' . 'дата/время' . Образец текста . Второй уровень . Третий уровень . Четвертый уровень . Пятый уровень . 'нижний колонтитул' . '#' .
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Ссылки http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/master01.htm -- 6.6 Кб -- 04.09.2006
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10996. http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/outline.htm
Заметки . Показ слайдов . Структура . ... Prague, August 16, 2006 . ...
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Ссылки http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/outline.htm -- 20.3 Кб -- 04.09.2006
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10997. Презентация PowerPoint
Prague, August 16, 2006 . To start a new GCVS edition (presumably an electronic one), combining the stars of the GCVS IV and Name Lists (and maybe eventually merged with automatic-survey variables), we need to revise the GCVS classification system. ... Our approach: the classification scheme must be simplified, more detailed classification should be given in specialized catalogs for particular types, but the GCVS classification should take into account new astrophysics. ...
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Ссылки http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/slide0007.htm -- 7.2 Кб -- 04.09.2006
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10998. Презентация PowerPoint
. Prague, August 16, 2006 . Examples of ASAS-3 light curves used by the GCVS team to improve astrophysical information in southern constellations show excellent prospects for a new, much improved edition of the GCVS
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Ссылки http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/slide0008.htm -- 6.1 Кб -- 04.09.2006
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10999. Презентация PowerPoint
Prague, August 16, 2006 . I am going to suggest the IAU Division V and Commission 27 a draft of a new GCVS classification scheme. ... It will also be available, after the GA, at the GCVS web site ( http://www.sai.msu.ru/groups/cluster/gcvs/ ) . We will start applying the scheme in the nearest future but are ready to take into account the future C27 suggestions, probably to be finally approved during the next GA of the IAU. ...
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Ссылки http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/slide0009.htm -- 6.0 Кб -- 04.09.2006
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11000. Презентация PowerPoint
Prague, August 16, 2006 . ... Large classes (groups of types) : . ... Eruptive variable stars . ... Pulsating variable stars . ... Rotating variable stars . ... Cataclysmic (explosive and nova-like) variables . ... Close binary eclipsing systems . ... Optically variable close-binary sources of strong variable X- ray radiation . ... These classes are just a way to group types; in our opinion, they can be kept if slightly better described ( e.g ., remove close from item 5, simplify item 6) ...
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Ссылки http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/slide0010.htm -- 8.4 Кб -- 04.09.2006
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