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361. http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/outline.htm

Заметки . Показ слайдов . Структура . ... Prague, August 16, 2006 . ...

[ Сохраненная копия ] Ссылки http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/outline.htm -- 20.3 Кб -- 04.09.2006
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362. http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/script.js

... 1 && GetHrefObj( gCurSld-1 ).mVis == 1 )|| ... GetNumSlds()) } function CloseWindow() { if( HideMenu() ) return ; var event = PPTSld.event; if( !IsFramesMode() event (event.keyCode==27 || event.keyCode==32 || event.type== click ) ) window.close( self ); CatchNumKeys( self, event ); } function Unload() { gIsEndShow=0; } function SetupEndShow() { gIsEndShow=1; PPTSld.document.body.scroll= no ; PPTSld.document.onkeypress=CloseWindow; PPTSld.document ...

[ Сохраненная копия ] Ссылки http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/script.js -- 25.6 Кб -- 04.09.2006
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363. 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. ...

[ Сохраненная копия ] Ссылки http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/slide0007.htm -- 7.2 Кб -- 04.09.2006
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364. 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

[ Сохраненная копия ] Ссылки http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/slide0008.htm -- 6.1 Кб -- 04.09.2006
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365. 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. ...

[ Сохраненная копия ] Ссылки http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/slide0009.htm -- 6.0 Кб -- 04.09.2006
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366. 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) ...

[ Сохраненная копия ] Ссылки http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/slide0010.htm -- 8.4 Кб -- 04.09.2006
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367. Презентация PowerPoint

Prague, August 16, 2006 . Our trial revision of the GCVS data for several southern constellations show that type changes are not needed for most stars. ... We suggest to add one more symbol combining types, in the cases when two or more classification options remain for the same star, for example, EC|Ell, EC|RR (here EC means a contact eclipsing binary, this is one of our suggestions from next slides). ... Moreover, it will simplify moving stars from the suspected-variable catalogue to the GCVS. ...

[ Сохраненная копия ] Ссылки http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/slide0011.htm -- 6.6 Кб -- 04.09.2006
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368. Презентация PowerPoint

. Prague, August 16, 2006 . Present classification : Suggested: . ACYG ACyg . BCEP, BCEPS BCep (BCEPS, after Jakate, seem . not justified) . CEP Cep . DCEP, DCEPS, CEP(B) DCep, DCep0, DCep1, DCepB01, . DCepB12 . Remark: 0 - fundamental, 1 - 1 st . overtone, 01 - fundamental plus . overtone, 12 - 1 st and 2 nd overtones. For non-beat Cepheids, it is safer . not to indicate the mode yet . PULSATING VARIABLES

[ Сохраненная копия ] Ссылки http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/slide0012.htm -- 8.3 Кб -- 04.09.2006
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369. Презентация PowerPoint

. Prague, August 16, 2006 . THANK YOU! . I think that good catalogues of variable stars are still needed and hope that our community will learn to handle the immense flow of information.

[ Сохраненная копия ] Ссылки http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/slide0013.htm -- 8.1 Кб -- 04.09.2006
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370. 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)

[ Сохраненная копия ] Ссылки http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/slide0017.htm -- 7.5 Кб -- 04.09.2006
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371. 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)

[ Сохраненная копия ] Ссылки http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/slide0018.htm -- 7.6 Кб -- 04.09.2006
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372. 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)

[ Сохраненная копия ] Ссылки http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/slide0019.htm -- 6.0 Кб -- 04.09.2006
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373. 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

[ Сохраненная копия ] Ссылки http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/slide0020.htm -- 7.6 Кб -- 04.09.2006
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374. 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)

[ Сохраненная копия ] Ссылки http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/slide0021.htm -- 6.6 Кб -- 04.09.2006
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375. 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

[ Сохраненная копия ] Ссылки http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/slide0022.htm -- 7.3 Кб -- 04.09.2006
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376. 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

[ Сохраненная копия ] Ссылки http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/slide0023.htm -- 7.6 Кб -- 04.09.2006
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377. 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)

[ Сохраненная копия ] Ссылки http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/slide0024.htm -- 7.8 Кб -- 04.09.2006
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378. Презентация PowerPoint

. Prague, August 16, 2006 . Present classification : Suggested: . ZAND Sym, NSym . CATACLYSMIC VARIABLES . AND OTHER STARS WITH OUTBURSTS (CONTINUED)

[ Сохраненная копия ] Ссылки http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/slide0025.htm -- 5.4 Кб -- 04.09.2006
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379. 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)

[ Сохраненная копия ] Ссылки http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/slide0026.htm -- 7.8 Кб -- 04.09.2006
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380. 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

[ Сохраненная копия ] Ссылки http://sai.msu.ru/groups/cluster/gcvs/future/iaupraha.files/slide0027.htm -- 7.0 Кб -- 04.09.2006
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