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The R.A.P.Project "Prosto o slozhnom" "Astro-ph za 2006 g." Nemnogo statistiki Predydushii vypusk (N177) Slovar' astroterminov Spisok missii i teleskopov Obzory UFN Stat'i SOZh ANKa Dnya 22.01.2008. Chernaya dyra v Omega Centavra 11.01.2008. Dvoinoe einshteinovskoe kol'co 06.08.2007. Kto eto tam tak bumknul? 14.03.2007. Taina kolec sverhnovoi 06.03.2007. BL Lac v zhestkom gamma Soderzhanie i bystryi perehod k razdelam obzora Stat'i nedeli "Luchshie iz luchshih" arxiv/0801.3175 Mnozhestvennye zvezdnye populyacii v galakticheskih sharovyh skopleniyah: nablyudatel'nye ukazaniya arxiv/0801.3230 Sverh-Zemlya s massoi 5 zemnyh, vrashayushayasya vokrug GJ 436?: preimushestva pochti skol'zyashih tranzitov Otdel'nye stat'i "Palomarskii poisk" - cifrovoi sinopticheskii obzor neba Kosmomikrofizika: zagadki i otkrytiya Mnozhestvennye zvezdnye populyacii v galakticheskih sharovyh skopleniyah: nablyudatel'nye ukazaniya Sverh-Zemlya s massoi 5 zemnyh, vrashayushayasya vokrug GJ 436?: preimushestva pochti skol'zyashih tranzitov ZEBRA 1.0 - rukovodstvo pol'zovatelya Vzveshivanie spokoinoi central'noi chernoi dyry v ellipticheskoi galaktike po dannym o rentgenovskom izluchenii gaza Sistematicheskie otkloneniya pri opredelenii nachal'noi funkcii mass iz-za razmera binov i nerazreshennyh sistem Komp'yuternoe modelirovanie obrazovaniya diskovyh galaktik3778 Peresmotr dalekogo budushego Solnca i Zemli Obzor oblasti galakticheskogo centra na neskol'kih dlinah voln na GBT Lekcii po kosmicheskim lucham vysokih energii Funkciya svetimosti galaktik i ee evolyuciya po dannym Chandra Slabaya yadernaya aktivnost' v blizkih spiral'nyh galaktikah Igolka v stoge sena - Gde iskat' odinochnye ostyvayushie neitronnye zvezdy Potencial'nye ob'ekty dlya Astro-G Iz razdela physics Preimushestva plazmennoi obrabotki tekstilya Ot Geizenberga do Einshteina? Vospominaniya i razmyshleniya o rozhdenii teorii strun Polnyi Arhiv predydushih vypuskov. Arhiv statei, voshedshih v vypuski s 01 iyulya 2002 g. po 31 marta 2003 g. Arhiv na 14.04.2006 odnim failom (36.9 Mb; *.tar.gz) gzip homepage Razdely arhiva (s aprelya 2003 g.): kosmologiya, neitrino, kosmicheskie luchi i gamma-astronomiya, galaktiki, AYaG, kvazary, nasha Galaktika, mezhzvezdnaya sreda, zvezdy, sverhnovye, ostatki sverhnovyh, chernye dyry, neitronnye zvezdy, linzirovanie, Solnce, ekzoplanety, Solnechnaya sistema, akkreciya, tesnye dvoinye sistemy, gamma-vspleski, gravitacionnye volny, mehanizmy izlucheniya, chislennoe modelirovanie, dinamika, mehanika metody obrabotki dannyh, MGD, metody nablyudenii, budushie nablyudatel'nye proekty, prochee. Poleznye astronomicheskie ssylki. Korotkoe esse ob elektronnyh preprintah. Obzornye stat'i v astro-ph 2001-2003 gg. Obsudit' na forume Scientific.RU Obsudit' na forume Zvezdocheta Obsudit' v bloge na Subscribe.ru Avtor proekta Sergei Popov Ranee uchastvovali: Mihail Prohorov Ekaterina Kasimova Diskussii po stat'yam Arhiva CosmoCoffee arXiv Blog Postav'te u sebya nashu knopku! Proekt razmeshen na saitah: Smotri takzhe diskussii i blogi: Informacionnye partnery Vy mozhet takzhe razmestit' na svoem saite nashu lentu obzorov Kniga avtora obzorov Novostnye lenty Novosti kosmonavtiki Novosti Nauchpopa Novosti ot UFN Informnauka Researcher@ Elementy.Ru Grani.Ru Perst Podpiska na rassylku obzorov na Subscribe.Ru Druzhestvennye rassylki: "Astronomiya segodnya" "Okno vo Vselennuyu" Spisok astrorassylok

Obzory preprintov astro-ph Vypusk N178 astro-ph za 22 - 31 yanvarya 2008 goda goda: izbrannye stat'i Referaty otdel'nyh statei arxiv:0801.3005 "Palomarskii poisk" - cifrovoi sinopticheskii obzor neba (The Palomar-Quest Digital Synoptic Sky Survey) Authors: S.G. Djorgovski, et al. Comments: 3 pages, 2 figures, macros included. To appear in refereed proceedings of "Hotwiring the Transient Universe 2007", eds. A. Allan, R. Seaman, and J. Bloom, Astron. Nachr. vol. 329, March, 2008 V korotkoi zametke opisan interesnyi obzor neba Palomar-Quest. Proekt nachalsya v 2003 godu i zakonchitsya v etom. Obzor vedetsya na 48-dyuimovom Shmidte s blokom PZS-matric (vmeste 161 Megapikselei). Za pervyi etap obzora (on uzhe zakonchen) polucheno izobrazhenie 15 000 kvadratnyh gradusov v neskol'kih fil'trah. Vtoroi etap (idet seichas) vedetsya v odnom (krasnom) fil'tre. Na etom etape vedetsya poisk sverhnovyh (a takzhe drugih tranzientov) i planet. Vazhno, chto etot obzor ispol'zuet protokoly, razrabotannye dlya Virtual'noi observatorii. miniobzor arxiv:0801.3028 Kosmomikrofizika: zagadki i otkrytiya (Astroparticle Physics: Puzzles and Discoveries) Authors: V. Berezinsky Comments: 13 pages, Invited talk at TAUP 2007 conference, September 2007, Sendai, Japan Interesnoe esse, posvyashennoe nekotorym zagadkam v kosmologii i rodstvennyh oblastyah. Osnovnoe vnimanie udeleno effektu Greizena-Zacepina-Kuz'mina (GZK) i problemam s lyambda-chlenom. miniobzor arxiv:0801.3175 Mnozhestvennye zvezdnye populyacii v galakticheskih sharovyh skopleniyah: nablyudatel'nye ukazaniya (Multiple Stellar Populations in Galactic GCs: Observational Evidence) Authors: Giampaolo Piotto Comments: 10 pages, Invited talk given at the Cefalu' 2007 Workshop "XXI Century Challenges for Stellar Evolution". To appear in Memorie della Societa' Astronomica Italiana, vol. 79/2, eds. S. Cassisi & M. Salaris Obychno schitaetsya, chto standartnoe, "horoshee" sharovoe skoplenie sostoit iz zvezd odnogo vozrasta i himicheskogo sostava. Odnako poslednie detal'nye fotometricheskii issledovaniya pokazyvayut nekotoroe raznoobrazie svoistv skoplenii. Vozmozhno, chto eto svyazano s tem, chto chast' skoplenii (kak, naprimer, Omega Centavra i M54 - dva iz shesti skoplenii, u kotoryh obnaruzheno raznoobrazie sostava) yavlyaetsya ostatkami karlikovyh galaktik, zahvachennyh nashei. Krome togo, massivnye sharovye skopleniya (chetyre drugih skopleniya - NGC 6388, NGC 1851, NGC 6441 i NGC 2808, takzhe kak i Omega Centavra i M54, yavlyayutsya massivnymi - massa bolee milliona solnechnyh), kak polagayut nekotorye avtory, mozhet zahvatyvat' zvezdy vo vremya svoego formirovaniya. arxiv:0801.3230 Sverh-Zemlya s massoi 5 zemnyh, vrashayushayasya vokrug GJ 436?: preimushestva pochti skol'zyashih tranzitov (A ~5 M_earth Super-Earth Orbiting GJ 436?: The Power of Near-Grazing Transits) Authors: Ignasi Ribas, Andreu Font-Ribera, Jean-Philippe Beaulieu Comments: 4 pages, 3 figures, submitted to The Astrophysical Journal Letters Srazu otmechu nalichie znaka voprosa v zagolovke. T.e., eto ne 100-procentnoe otkrytie, a "sil'noe ukazanie na". Tem ne menee. Tem ne menee, eto ukazanie na otkrytie legkoi (pyat' zemnyh mass) planety vokrug zvezdy glavnoi posledovatel'nosti (pravda, eto dovol'no tusklyi krasnyi karlik spektral'nogo klassa M). Zapodozrit' sushestvovanie legkoi planety avtory smogli po otkloneniyam v dvizhenii bolee massivnoi (s massoi poryadka neptunovoi) planety. Massivnaya planeta - tranzitnaya. Otsyuda i vtoraya polovina zagolovka. Imenno "skol'zyashii" harakter prohoda massivnoi planety po disku zvezdy pozvolil obnaruzhit' (tochnee - zapodozrit') malye otkloneniya, vozmozhno vyzyvaemye legkoi planetoi. Obsudit' v ZhZh-soobshestve ru_astroph. Obsudit' na Astroforume v Nauchnoi panorame. arxiv:0801.3275 ZEBRA 1.0 - rukovodstvo pol'zovatelya (ZEBRA 1.0 -- User manual) Authors: R. Feldmann Comments: 33 pages, 3 Figures, 7 Tables. ZEBRA - Zurich Extragalactic Bayesian Redshift Analyzer. Eto otkrytaya programma, pozvolyayushaya provodit' massovye opredeleniya krasnyh smeshenii vnegalakticheskih ob'ektov po fotometricheskim dannym. Stat'ya yavlyaetsya rukovodstvom k etoi programme. arxiv:0801.3461 Vzveshivanie spokoinoi central'noi chernoi dyry v ellipticheskoi galaktike po dannym o rentgenovskom izluchenii gaza (Weighing the Quiescent Central Black Hole in an Elliptical Galaxy with X-ray Emitting Gas) Authors: Philip J. Humphrey et al. Comments: 12 pages, 6 figures, submitted to ApJ Gigantskaya ellipticheskaya galaktika NGC4649 nahoditsya v centre gruppy galaktik. Mozhno bylo by ozhidat', chto v galakticheskom centre nahoditsya sverhmassivnaya chernaya dyra, no nikakoi aktivnosti, svyazannoi s nei, ne nablyudaetsya. Tem ne menee, svoei massoi dyra sebya vydaet. Nablyudeniya zvezdnoi kinematiki uzhe pozvolili sdelat' ocenku massu chernoi dyry. A v etoi stat'e avtory ispol'zuyut eshe odin metod dlya "vzveshivaniya" chernoi dyry. Oni nablyudayut goryachii gaz v galaktike po ego rentgenovskomu izlucheniyu. V potenciale galaktiki bez central'nogo massivnogo ob'ekta gaz dolzhen byt' holodnee v central'nyh oblastyah. Ponachalu i v NGC4649 temperatura gaza spadaet ot 20 kpk do ~1 kpk ot centra. No detal'nye issledovaniya gaza vnutri 200 pk ot centra galaktiki pokazali, chto tam nachinaetsya rost temperatury. Eto mozhno ob'yasnit' nalichiem ochen' massivnoi chernoi dyry. Bolee togo, esli sdelat' razumnoe predpolozhenie o gidrostaticheskom ravnovesii, to mozhno sdelat' ocenku massy dyry. Dlya NGC4649 ona poluchaetsya ravnoi primerno 3 milliardam mass Solnca. Eta ocenka sovpadaet so sdelannoi po kinematike zvezd. Dannoe sovpadenie pozvolyaet avtoram stat'i perevernut' argumentaciyu i govorit' o tom, chto my imeem podtverzhdenie togo, chto gaz nahoditsya v gidrostaticheskom ravnovesii. arxiv:0801.3778 Sistematicheskie otkloneniya pri opredelenii nachal'noi funkcii mass iz-za razmera binov i nerazreshennyh sistem (IMF biases created by binning and unresolved systems) Authors: J. Maiz Apellniz Comments: : 6 pages, 10 figures, to appear in "Young massive clusters, initial conditions and environments" Nebol'shoe izlozhenie dvuh bol'shih rabot. Avtor analiziruet, chto meshaet tochnomu opredeleniyu funkcii mass. Pristal'no rassmotreny dva momenta: razmer binov (po masse) i rol' kratnyh zvezd (kak fizicheskih, tak i opticheskih). Tam gde chto-to mozhno ispravit', avtor predlagaet puti korrekcii opredelennoi funkcii mass. V nekotoryh sluchayah (naprimer, kogda na izobrazhenii "slipaetsya" bol'shoe chislo zvezd) nichego sdelat' uzhe nel'zya. obzor arxiv:0801.3845 Komp'yuternoe modelirovanie obrazovaniya diskovyh galaktik (The formation of disk galaxies in computer simulations) Authors: Lucio Mayer, Fabio Governato, Tobias Kaufmann Comments: 41 pages, 15 figures, Invited Review accepted for publication on Advanced Science Letters. Obzor posvyashen modelirovaniyu (a, stalo byt', i ponimaniyu) processa obrazovaniya diskovyh galaktik. Poskol'ku problema daleka ot okonchatel'nogo resheniya, obzor soderzhit v sebe intrigu, chto delaet chtenie interesnym. arxiv:0801.4031 Peresmotr dalekogo budushego Solnca i Zemli (Distant future of the Sun and Earth revisited) Authors: Klaus-Peter Schroder, Robert C. Smith Comments: 10 pages, MNRAS 2008, in print (accepted Jan. 23rd, 2008) Na osnove novyh modelei zvezdnoi evolyucii avtory rassmatrivayut dalekoe budeshee Solnca i okruzhayushih ego planet, v chastnosti i Zemli. Krome togo, rezul'taty prilagayutsya k ozhidaemym svoistvam planet vokrug belyh karlikov. V budushem Solnce budet sbrasyvat' veshestvo. Eto budet privodit' k rasshireniyu planetnyh orbit. S drugoi storony, esli planeta vse-taki okazhetsya slishkom blizko k rasshirevsheisya zvezde, to planeta budet tormizit'sya za schet vozdeistviya vneshnih sloev zvezdy (krome togo, vazhny i prilivnye sily). V itoge planeta po spirali budet padat' na zvezdu. Sootvetstvenno, est' nekotoroe kriticheskoe rasstoyanie: planety, nahodyashiesya (kogda zvezda nahoditsya na stadii glavnoi posledovatel'nosti, t.e. "seichas" v sluchae Solnechnoi sistemy) blizhe nekotorogo rasstoyaniya, upadut na zvezdu, kogda ona stanet gigantom. Po ocenkam avtorov dlya Solnca eto rasstoyanie ravno 1.15 astronomicheskoi edinicy. T.e., oni predrekayut Zemle dovol'no pechal'noe budushee. "Eto ochen' ogorchaet". Pravda, sluchitsya eto tol'ko cherez 7 s hvostikom milliardov let. Krome togo, avtory issleduyut i drugie aspekty budushei evolyucii Solnca. V chastnosti, oni polagayut, chto nasha zvezda ne dast krasivoi planetarnoi tumannosti (hotya sbros veshestva, razumeetsya, budet znachitel'nym). V zaklyuchenie podcherknu, chto konechno zhe modeli zvezdnoi evolyucii (dazhe dlya Solnca) poka ne dostigli toi tochnosti, chtoby pisat' chto-to v duhe "astronomy dokazali, chto..." (kstati, o perspektivah utochneniya modelei Solnca s pomosh'yu gelioseismologii mozhno prochest' zdes' arxiv:0801.4213). Predstavlen rezul'tat, poluchennyi v ramkah nekotoroi modeli. Kachestvenno, tam vse verno. No vot poruchit'sya za chisla vrode "1.15 a.e." poka mozhno lish' s opredelennoi stepen'yu uverennosti. Obsudit' v ZhZh-soobshestve ru_astroph. Obsudit' na Astroforume v Nauchnoi panorame. arxiv:0801.4294 Obzor oblasti galakticheskogo centra na neskol'kih dlinah voln na GBT (GBT Multiwavelength Survey of the Galactic Center Region) Authors: C. J. Law et al. Comments: Accepted to ApJS. 40 pages, 46 figures, 8 tables (emulate apj style) Predstavleny rezul'taty radioobzora na volnah 3.5, 6. 20 i 90 santimetrov oblasti centra Galaktiki. Razmer oblasti 4 na 1 gradus. Obzor proveden na 100-metrovom Green Bank Telescope. Avtory pishut, chto na dlinah 3.5 i 6 santimetrov eto samyi glubokii obzor dannoi oblasti. obzor arxiv:0801.4376 Lekcii po kosmicheskim lucham vysokih energii (Lecture notes on high energy cosmic rays) Authors: M. Kachelriess Comments: 82 pages, prepared for the 17th Jyvaskyla Summer School Obzory i lekcii po kosmicheskim lucham poyavlyayutsya regulyarno, i ne na vse ih nih ya obrashayu vashe vnimanie. Dannye lekcii menya zainteresovali tem, chto zdes' akkuratno privedeny mnogie bazovye veshi. 80 stranic teksta - eto nemalo, i avtor smog raz'yasnit' mnogie ponyatiya, kotorye obychno v obzorah ne razzhevyvayutsya. arxiv:0801.4381 Funkciya svetimosti galaktik i ee evolyuciya po dannym Chandra (The galaxy luminosity function and its evolution with Chandra) Authors: P. Tzanavaris, I. Georgantopoulos Comments: 11 pages, Accepted for publication in A&A Avtory rassmotreli vyboru iz primerno sotni normal'nyh (t.e. bez aktivnogo yadra) galaktik rannego tipa (ellipticheskih) i takogo zhe kolichestva galaktik pozdnego tipa (spiral'nye i nepravil'nye) vplot' do krasnogo smesheniya 1.4. Ih interesoval vopros ob evolyucii rentgenovskoi svetimosti etih galaktik. Rentgenovskoe izluchenie ellipticheskih galaktik v osnovnov opredelyaetsya goryachim gazom s nebol'shoi dobavkoi vklada ot malomassivnyh dvoinyh. Dlya galaktik pozdnih tipov dvoinye gorazdo vazhnee, prichem bol'shaya dolya izlucheniya svyazana s massivnymi dvoinymi, kotoryh v ellipticheskih galaktikah prakticheski net. Rezul'taty takovy. Dlya galaktik pozdnih tipov avtory obnaruzhili sil'nuyu evolyuciyu funkcii svetimosti s krasnym smesheniem v sootvetstvii so stepennym zakonom ~(1+z)k, gde k poryadka 2-3. Dlya galaktik rannego tipa sil'noi evolyucii net. No, poskol'ku na z>0.5 v ih vyborke dominiruyut galaktiki pozdnih tipov, to dlya summarnoi evolyucii vseh galaktik vmeste rezul'tat poluchaetsya pochti takoi zhe, kak dlya pozdnih. arxiv:0801.4382 Slabaya yadernaya aktivnost' v blizkih spiral'nyh galaktikah (Low-Level Nuclear Activity in Nearby Spiral Galaxies) Authors: Himel Ghosh et al. Comments: 38 pages, 10 figures, submitted to ApJ Avtory rasmatrivayut blizkie spiral'nye galaktiki s cel'yu vyyavit' v nih otnositel'no legkie sverhmassivnye chernye dyry po ih rentgenovskomu izlucheniyu. Napomnyu, chto schitaetsya, chto lyubaya galaktika s zametnoi sfericheskoi sostavlyayushei (baldzhem) soderzhit v sebe sverhmassivnuyu chernuyu dyru. Chem massivnee baldzh - tem tyazhelee i dyra. U spiral'nyh galaktik baldzhi neveliki, poetmou i dyry dolzhny byt' legkimi (v nashei, napomnyu, massy dyry okolo 2-3 millionov solnechnyh mass; sravnite s milliardami v bol'shih ellipticheskih galaktikah). Avtory ispol'zovali dannye Chandry dlya shesti galaktik, vidimyh plashmya. Dlya vseh shesti naideny yadernye rentgenovskie istochniki. T.e., pohozhe vse shest' yavlyayutsya aktivnymi. arxiv:0801.4567 Igolka v stoge sena - Gde iskat' odinochnye ostyvayushie neitronnye zvezdy (The needle in the haystack - Where to look for more isolated cooling neutron stars) Authors: The needle in the haystack - Where to look for more isolated cooling neutron stars Authors: B. Posselt, S.B. Popov, F. Haberl, J. Truemper, R. Turolla, R. Neuhaeuser Comments: 14 pages, 9 figures, accepted by A&A Ya redko pishu o svoih rabotah. Sobstvenno, eto vsego pyatyi sluchai za shest' let. No tut uderzhat'sya ne mogu: slishkom uzh dolgo my dobiralis' do prinyatiya stat'i v pechat'. Vo-pervyh, v rabote predstavlena novaya versiya programmy populyacionnogo sinteza dlya rascheta evolyucii blizkih ostyvayushih neitronnyh zvezd. Vo-vtoryh, rezul'taty raboty ispol'zuyutsya dlya otveta na vopros o tom, gde iskat' novyh kandidatov. Ved' seichas Velikolepnaya semerka na kone. No esli za pervye pyat' let issledovaniya etih ob'ektov udalos' otkryt' semerku, to za sleduyushie pyat' - ni odnogo. V-tret'ih, v final'noi chasti stat'i obsuzhdayutsya "netradicionnye" idei po poisku novyh blizkih ostyvayushih neitronnyh zvezd. arxiv:0801.4863 Potencial'nye ob'ekty dlya Astro-G (Potential Targets for ASTRO-G In-Beam Phase-Referencing) Authors: S. Frey, K.E. Gabanyi Comments: 3 pages; proceedings of the symposium "Approaching Micro-Arcsecond Resolution with VSOP-2: Astrophysics and Technology" (ISAS/JAXA, Sagamihara, Japan, 3-7 Dec 2007). Astronomical Society of the Pacific Conference Series, eds. Hagiwara Y., Fomalont E.B., Tsuboi M., Murata Y. ASTRO-G - budushii yaponskii sputnik. On takzhe izvesten kak VSOP-2. VSOP - The VLBI Space Observatory Programm. Eto programma, v ramkah kotoroi sozdaetsya radiointerferometr s kosmicheskim elementom, t.e. s antennoi na sputnike. Pervyi apparat - HALCA - uzhe otrabotal (s 1997 po 2003 god). Vtoroi apparat - ASTRO-G - planiruetsya k zapusku v 2012 godu. Kraine polezno za dolgo do zapuska nachinat' publichnoe obsuzhdenie apparata, ego vozmozhnoi nauchnoi programmy, optimizacii tehnicheskih detalei i tp. Dlya eto, v chastnosti, provodyatsya special'nye mezhdunarodnye konferencii. Est' takie konferencii i v ramkah razrabotki ASTRO-G. Odna iz nih - "Approaching Micro-Arcsecond Resolution with VSOP-2: Astrophysics and Technology" proshla v konce proshlogo goda. Na stranice konferencii mozhno skachat' prezentacii. No budut i materialy. Stat'i dlya etogo sbornika potihon'ku vykladyvayutsya v Arhiv. V stat'e, kotoraya posluzhila povodom upomyanut' sputnik i konferenciyu, rech' kak raz idet ob otbore ob'ektov dlya nablyudeniya v ramkah novoi missii. Krome etogo, v poslednem yanvarskom vypuske poyavilos' eshe dve raboty iz materialov konferencii po VSOP-2: High-Redshift Quasars at the Highest Resolution: VSOP Results, The Need For High Resolution In Studies Of The 3-D Magnetic Field Structure Of AGN Jets. Ochevidno, budut poyavlyat'sya i drugie podobnye stat'i. My budem starat'sya hotya by perechislit' interesnye (dlya shirokoi publiki) stat'i, poyavivshiesya v razdele physics (vklyuchaya cross-listing). arxiv:0801.3727 Preimushestva plazmennoi obrabotki tekstilya (Plasma treatment advantages for textiles) Authors: Amelia Sparavigna Comments: 16 pages Po-moemu ochen' interesnaya stat'ya. ne berus' sudit' ob original'nyh rezul'tatah, predstavlennyh avtorom. No obzor togo, kak plazmennaya obrabotka izmenyaet svoistva tkanei i poverhnostei ochen' interesen. arxiv:0801.4694 Ot Geizenberga do Einshteina? Vospominaniya i razmyshleniya o rozhdenii teorii strun (From Heisenberg to Einstein? Recollections and afterthoughts on the birth of string theory) Authors: Renato Musto Comments: 7 pages, Contribute to the collective volume "The birth of String Theory", edited by A. Cappelli, E. Castellani, F. Colomo and P. Di Vecchia Korotkaya zametka, v kotoroi odin iz uchastnikov sobytii (Renato Musto - soavtor dvuh top-citiruemyh rabot po teorii strun, napisannyh v seredine 70-h) vspominaet i razmyshlyaet o samom rannem etape v zhizni teorii strun i o tom, chto etomu etapu neposredstvenno predshestvovalo. Horoshaya ssylka nomer 12. Vernut'sya k nachalu stranicy

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