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The R.A.P.Project "Prosto o slozhnom" "Astro-ph za 2006 g." Nemnogo statistiki Predydushii vypusk (N176) Slovar' astroterminov Spisok missii i teleskopov Obzory UFN Stat'i SOZh ANKa Dnya 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/0801.1555 Sloanovskii obzor linz. VI: Otkrytie i analiz dvoinogo kol'ca Einshteina arxiv/0801.2782 Ukazaniya po dannym Dzhemini i Kosmicheskogo teleskopa im. Habbla na sushestvovanie chernoi dyry promezhutochnoi massy v Omega Centavra arxiv/0801.2944 Fizika vrasheniya v zvezdnyh modelyah Otdel'nye stat'i Registraciya i klassifikaciya tranzientov Sloanovskii obzor linz. VI: Otkrytie i analiz dvoinogo kol'ca Einshteina Nukleosintez v zvezdnyh vspyshkah Registraciya bleska zvezd ot okeanov na dalekih planetah CESAM: svobodnaya programma dlya rascheta zvezdnoi evolyucii The World Space Observatory (WSO-UV) - tekushee sostoyanie ARTEMiS (Automated Robotic Terrestrial Exoplanet Microlensing Search) - predlagaemaya ekspertnaya sistema, osnovannaya na sovmestnom poiske s massoi poryadka zemnoi i menee Raspredelenie semeistv asteroidov po forme - ukazanie na evolyuciyu za schet slabyh stolknovenii Obrazovanie planet zemnogo tipa v drugih planetnyh sistemah Anizotropiya relikta: otkrytie i primenenie Strunnaya kosmologiya: obzor Vysokotochnyi taiming PSR J0437-4715: dostovernoe rasstoyanie do pul'sara, vysokaya massa i predel na variaciyu n'yutonovskoi konstanty Pul'sarnye tumannosti v epohu Chandry Rasstoyanie do centra Galaktiki po cefeidam populyacii II i zvezdam tipa RR Liry Ukazaniya po dannym Dzhemini i Kosmicheskogo teleskopa im. Habbla na sushestvovanie chernoi dyry promezhutochnoi massy v Omega Centavra Fizika vrasheniya v zvezdnyh modelyah Radiotranzienty: sovremennaya i gryadushaya kartiny Iz razdela physics Etiketki i fizika: razvitie novyh metodov markirovki kak novoe mnogoobeshayushee pole dlya prikladnoi fiziki 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 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 N177 astro-ph za 10 - 21 yanvarya 2008 goda goda: izbrannye stat'i Referaty otdel'nyh statei arxiv:0801.1503 Registraciya i klassifikaciya tranzientov (Transient Detection and Classification) Authors: Andrew C. Becker Comments: 4 pages. In Proceedings of Hot-wiring the Transient Universe (HTU) 2007. To be published in Astronomische Nachrichten, March 2008 V stat'e rech' idet o budushih nablyudeniyah opticheskih tranzientov (sm., naprimer, saity proektov PAN-STARS, LSST). Ob'em stat'i nevelik, no v perechen' tranzientov popali i iskusstvennye sputniki, i tela Solnechnoi sistemy, i ekzoplanety, i vspyhivayushie zvezdy, i mikrolinzirovanie, i obychnye peremennye zvezdy, i sverhnovye, i opticheskie poslesvecheniya gamma-vspleskov. Samaya vazhnaya sostavlyayushaya stat'i - eto obsuzhdenie organizacii alertov (t.e. bystryh soobshenii o tranziente) i posleduyushih nablyudenii. Syuda zhe otnosyatsya i problemy klassifikacii. arxiv:0801.1555 Sloanovskii obzor linz. VI: Otkrytie i analiz dvoinogo kol'ca Einshteina (The Sloan Lens ACS Survey. VI: Discovery and analysis of a double Einstein ring) Authors: Raphael Gavazzi et al. Comments: 15 pages Otkryt krasiveishii sluchai linzirovaniya: dvoinoe einshteinovskoe kol'co. Dlya etogo nado, chtoby tri galaktiki okazalis' pochti na odnoi pryamoi. Izobrazhenie dvoinogo kol'ca. Hotya linza pervonachal'no byla otkryta po dannym Sloanovskogo obzora, no kachestvennoe izobrazhenie polucheno uzhe Kosmicheskim teleskopom. Sprava pokazano uvelichennoe izobrazhenie, s kotorogo ubrali galaktiku-linzu. Galaktika, igrayushaya rol' linzy, nahoditsya na krasnom smeshenii z=0.222. Vnutrennee kol'co - na z=0.609. Gde nahoditsya vtoroe kol'co tochno neizvestno, no skoree vsego eto z=2-5. V principe, linzy s dvumya galaktikami-istochnikami dolzhny vstrechat'sya ne tak uzh redko: raz na 40-80 sluchaev sil'nogo linzirovaniya. A sil'noe linzirovanie vstrechaetsya primerno raz na 200 massivnyh galaktik rannih tipov. Tem ne menee, krasivoe dvoinoe kol'co einshteina naideno vpervye. Ved' dlya polucheniya dvuh einshteinovskih kolec nado, chtoby vyravnivanie galaktik na odnoi pryamoi bylo ochen' horoshim. Neudivitel'no, chto sdelano eto v ramkah Sloanovskogo cifrovogo obzora neba. Prichem, avtoram povezlo: stol' redkii zver' popalsya posle obnaruzheniya primerno 90 linz. Razumeetsya, bolee dalekaya galaktika linziruetsya ne tol'ko sobstvenno linzoi na z=0.222), no i vtorym (bolee blizkim, z=0.609) istochnikom, poetomu vtoroe kol'co shire. Tak chto situaciya neprostaya. i avtory detal'no ee modeliruyut. Obsudit' v ZhZh-soobshestve ru_astroph. Obsudit' na Astroforume v Nauchnoi panorame. miniobzor arxiv:0801.1777 Nukleosintez v zvezdnyh vspyshkah (Nucleosynthesis in stellar flares) Authors: V. Tatischeff, J.-P. Thibaud, I. Ribas Comments: 12 pages, 3 figures, contribution to the Proceedings of the XIXemes Rencontres de Blois, Matter and energy in the Universe, Blois, France, May 2007 Litii obrazuetsya v hode pervichnogo nukleosinteza v molodoi vselennoi. V zvezdah litii ne proizvoditsya v cepochkah temroyadernyh reakcii, za schet kotoryh zvezdy svetyat. Poetomu v osnovnom ves' litii vo vselennoi pervichnyi. Odnako, est' interesnaya hitrost'. Vo vspyshkah na zvezdah mozhet obrazovyvat'sya nemnozhko litiya, sovsem chut'-chut'. V masshtabah vselennoi eto kraine malyi vklad. Odnako soderzhanie litiya zachastuyu opredelyaetsya imenno po nablyudeniyam zvezd. Poetomu dazhe nebol'shaya dobavka litiya vo vneshnih sloyah zvezdy mozhet vvesti issledovatelya v zabluzhdenie, t.k. on mozhet zakrichat' "Evrika!", ne vyliv sebe na golovu vedro holodnoi vody reshit', chto on nashel argument v pol'zu vysokogo soderzhaniya litiya vo vselennoi vcelom (ili v pol'zu togo, chto litiya bylo mnogo lokal'no v tom gazovom oblake, iz kotorogo formirovalas' nablyudaemaya zvezda). Avtory detal'no razbirayut vozmozhnoe uvelicheniya soderzhaniya litiya v poverhnostnyh sloyah zvezd za schet generacii etogo elementa v rezul'tate vspyshek. Kstati, naibolee interesny (s kosmologicheskoi tochki zreniya) nablyudeniya litiya na karlikovyh zvezdah v galo nashei Galaktiki, t.k. malomassivnye zvezdy dolgo zhivut, i, sootvetstvenno, seichas po nim my mozhem uznat' himicheskii sostav na zare formirovaniya nashei zvezdnoi sistemy. Tak vot, kak raz na karlikovyh zvezdah, kak vse pomnyat, vspyshki v osnovnom i proishodyat. Tak chto problema ves'ma aktual'na i ser'ezna. arxiv:0801.1852 Registraciya bleska zvezd ot okeanov na dalekih planetah (Detecting the Glint of Starlight on the Oceans of Distant Planets) Authors: D.M. Williams, E. Gaidos Comments: 41 pages, 7 figures. Icarus in press Avtory utverzhdayut, chto planety s okeanami i atmosferami tipa zemnoi mozhno budet vydelyat' po krivym bleska, t.k. svet ot ih solnca budet blikovat' na poverhnosti okeana. Ideya ochen' krasivaya i avtory ee detal'no razvivayut. Obsudit' v ZhZh-soobshestve ru_astroph. Obsudit' na Astroforume v Nauchnoi panorame. arxiv:0801.2019 CESAM: svobodnaya programma dlya rascheta zvezdnoi evolyucii (CESAM: a free code for stellar evolution calculations) Authors: Pierre Morel, Yveline Lebreton Comments: 13 pages, 1 figure, accepted for publication in Astrophysics & Space Science, ESTA/CoRoT Volume Podrobno opisyvaetsya paket programm dlya rascheta zvezdnoi evolyucii. Raschety odnomernye. Ne uchityvaetsya vyrozhdenie elektronov. Navernoe, mnogiem budet interesno takzhe prosmotret' stat'yu arxiv:0801.2022. V nei avtor rassuzhdaet o perspektivah mikrosekundnoi zvezdnoi astrometrii (na takom urovne budet rabotat' sputnik GAIA). Okazyvaetsya, eta zadacha brosaet vyzov i zvezdnym modelyam. Kogda astrometriya vyidet na mikrosekundnyi uroven', odnomernymi modelyami budet uzhe ne oboitis'. arxiv:0801.2080 The World Space Observatory (WSO-UV) - tekushee sostoyanie (The World Space Observatory (WSO-UV) - Current status) Authors: Michela Uslenghi et al. Comments: 6 pages, 5 figures; Chinese Journal for Astronomy and Astrophysics (ChJAA), in press. Invited talk at the Frascati Workshop 2007 Vulcano (Italy), May 28 - June 2 "Multifrequency Behaviour Of High Energy Cosmic Sources" WSO-UV - eto to, chto kogda-to bylo izvestno kak Spektr-UF. Seichas (po nauchnoi chasti) eto proekt v osnovnom ne rossiiskii. Odnako imenno za Rossiei sozdanie 170-santimetrovogo teleskopa i sobstvenno sputnika, a takzhe zapusk. Priemnaya apparatura budet sozdavat'sya v Germanii, Kitae i Italii. Zapusk namechaetsya na 2011 god. Sozdateli nadeyutsya, chto apparat prorabotaet okolo 10 let. V stat'e opisyvayutsya osnovnye parametry sputnika i ustanovlennoi na nem apparatury. Sm. takzhe arxiv:0801.2039. arxiv:0801.2162 ARTEMiS (Automated Robotic Terrestrial Exoplanet Microlensing Search) - predlagaemaya ekspertnaya sistema, osnovannaya na sovmestnom poiske s massoi poryadka zemnoi i menee (ARTEMiS (Automated Robotic Terrestrial Exoplanet Microlensing Search) - A possible expert-system based cooperative effort to hunt for planets of Earth mass and below) Authors: M. Dominik et al. Comments: 4 pages with 2 eps figures embedded. Accepted for publication in Astronomische Nachrichten as part of the Proceedings of the Joint VOEvent & HTN Workshop "Hot-wiring the Transient Universe" held in Tucson, Arizona (US), June 4-7 2007 Napomnyu, chto poka samaya legkaya planeta (s massoi poryadka 5 zemnyh) byla obnaruzhena metodom mikrolinzirovaniya. Zdes', pravda, nuzhno sdelat' odin kommentarii o metode. My govorim o mikrolinzirovanii, kogda odna zvezda linziruetsya drugoi (ili analogichnym ob'ektom: belym karlikom, neitronnoi zvezdoi, chernoi dyroi, burym karlikom i tp.). Sootvetstvenno, uchenye sledyat odnovremenno za millionami zvezd-istochnikov. Esli pryamo pered odnoi iz nih proletit zvezda-linza, to my uvidim vozrastanie bleska zvezdy-istochnika. Esli u linzy est' sputnik (planeta), to na krivoi bleska budet harakternyi pichok. Analiziruya krivuyu bleska mozhno poluchit' raspredelenie veroyatnostei dlya parametrov linzy (i ee sputnika, esli on est'). No kraine redko udaetsya obnaruzhit' samu linzu! Tak chto nesmotrya na svoyu silu metod mikrolinzirovaniya, v smysle poiska ekzoplanet, imeet i sushestvennye nedostatki: i zvezda-linza i ee sputnik chashe vsego ne nablyudayutsya posle sobytiya mikrolinzirovaniya, a parametry ne opredelyayutsya dostatochno dostoverno. Tem ne menee..... Tem ne menee, v obozrimom budushem tol'ko etot metod mozhet pozvolit' nabrat' bol'shuyu statistiku po legkim planetam. A dlya etogo nado mnogo nablyudat'. A dlya etogo nuzhno mnogo teleskopov-robotov, sovmestnye usiliya i horoshaya obrabotka dannyh. Vot eto-to i yavlyaetsya predmetom stat'i. Vozmozhno, chto i sami zvezdy-linzy udast'sya "vyhvatyvat'". arxiv:0801.2389 Raspredelenie semeistv asteroidov po forme - ukazanie na evolyuciyu za schet slabyh stolknovenii (The shape distribution of asteroid families -- evidence for evolution driven by small impacts) Authors: Gyula M. Szabo, Laszlo L. Kiss Comments: Accepted by Icarus. 22 pages, 1 table, 6 figures, 31 figure panels Issledovav krivye bleska bolee 11 tysyach asteroidov, avtory prishli k vyvodu, chto s vozrastom forma etih nebesnyh tel izmenyaetsya. Oni stanovyatsya bolee kruglymi. Vidimo, eto proishodit na schet neslishkom sil'nyh stolknovenii, kotorye ne razrushayut asteroidy, a ih "obtesyvayut". arxiv:0801.2560 Obrazovanie planet zemnogo tipa v drugih planetnyh sistemah (Terrestrial Planet Formation in Extra-Solar Planetary Systems) Authors: Sean N. Raymond Comments: 19 pages, 5 figures. To appear in the proceedings of IAU Symposium 249: Exoplanets: Detection, Formation and Dynamics, held in Suzhou, China, Oct 22-26 2007 Stat'ya posvyashena formirovaniyu zemnopodobnyh planet. Na 2-6 stranicah avtor privodit obzor sovremennoi modeli etogo processa. Zatem on perehodit k poluobzornomu izlozheniyu svoih (i soavtorov) rezul'tatov. Oni tozhe ves'ma interesny, no ya obrashayu vashe vnimanie na stat'yu v pervuyu ochered' imenno radi obzora, davaemogo v razdele 2. miniobzor arxiv:0801.2563 Anizotropiya relikta: otkrytie i primenenie (CMB Anisotropies: Their Discovery and Utilization) Authors: George F. Smoot Comments: 13 pages, 2 figures, A Century of Cosmology' held at San Servolo, Venice Prakticheski populyarnyi obzor po anizotropii reliktovogo izlucheniya. Opisana i istoriya issledovanii i otkrytii, i to "zachem eto nuzhno" v kosmologii, nu i, konechno zhe, chto eshe predstoit sdelat' na budushih eksperimentah. "Istoricheskii" podhod pomogaet ponyatnee vse izlozhit', tak chto stat'ya poluchaetsya ochen' dostupnaya. obzor arxiv:0801.2951 Strunnaya kosmologiya: obzor (String Cosmology: A Review) Authors: Liam McAllister, Eva Silverstein Comments: 55 pages Bolee ob'emnyi i menee dostupnyi obzor po kosmologii. Hotya formul ne tak uzh mnogo. Tak chto nadezhda razobrat'sya est' i u teh, kto ne zanimaetsya etoi oblast'yu. arxiv:0801.2589 Vysokotochnyi taiming PSR J0437-4715: dostovernoe rasstoyanie do pul'sara, vysokaya massa i predel na variaciyu n'yutonovskoi konstanty (Precision timing of PSR J0437-4715: an accurate pulsar distance, a high pulsar mass and a limit on the variation of Newton's gravitational constant) Authors: J.P.W. Verbiest et al. Comments: 19 pages, 4 figures, accepted for publication in The Astrophysical Journal Pul'sar PSR J0437-4715 - blizhaishii millisekundnyi pul'sar. Ego nablyudayut s 1993 goda. Kompan'onom neitronnoi zvezdy yavlyaetsya belyi karlik. Sistema horosho izuchena, i v dannoi stat'e avtory predstavlyayut svezhie rezul'taty po opredeleniyu mnogih parametrov. S tochki zreniya fiziki, pozhalui, naibolee interesna ocenka massy neitronnoi zvezdy: 1.76+/-0.2 solnechnyh. Tut sushestvenno to, chto dlya deistvitel'no horosho izuchennyh sistem (u etoi, naprimer, tochno izvestno naklonenie orbity, rasstoyanie i tp.) eto samaya vysokaya massa. A imenno vysokie znacheniya mass ogranichivayut uravneniya sostoyaniya veshestva pri vysokoi plotnosti. obzor arxiv:0801.1602 Pul'sarnye tumannosti v epohu Chandry (Pulsar Wind Nebulae in the Chandra Era) Authors: O. Kargaltsev, G. G. Pavlov Comments: 15 pages, 5 tables, 10 figures. To appear in the proceedings of "40 Years of Pulsars: Millisecond Pulsars, Magnetars, and More", August 12-17, 2007, McGill University, Montreal, Canada V poslednie gody bol'shoe vnimanie specialistov privlekayut t.n. pul'sarnye tumannosti. Rabotayushii pul'sar daet potok chastic, kotorye vzaimodeistvuyut s okruzhayushim veshestvom. V itoge voznikaet specificheskoe obrazovanie. Blagodarya vysokomu uglovomu razresheniyu rentgenovskogo teleskopa Chandra udaetsya izuchat' mnogie iz etih tumannostei v melkih podrobnostyah. Krome togo, razvitie nazemnoi gamma-astronomii (H.E.S.S., MAGIC, ...) daet vozmozhnost' nablyudat' eti ob'ekty na TeVnyh energiyah. T.e., idet bol'shoi potok dannyh, nu i teoretiki ne sidyat, slozhiv v ruki. Tak chto est' chto obozret', chto avtory i delayut. Est' krasivye kartinki. arxiv:0801.2652 Rasstoyanie do centra Galaktiki po cefeidam populyacii II i zvezdam tipa RR Liry (The distance to the Galactic Centre based on Population-II Cepheids and RR Lyrae stars) Authors: M.A.T. Groenewegen, A. Udalski, G. Bono Comments: 8 pages, A&A accepted V rasstoyanii do centra Galaktiki ostaetsya nekotoraya neopredelennost'. Est' rekomendovannoe Mezhdunarodnym astronomicheskim soyuzom znachenie 8.5 kpk. Est' storonniki "korotkoi shkaly". Soglasno etoi modeli rasstoyanie okazyvaetsya procentov na 10-20 men'she. Postoyanno poyavlyayutsya novye raboty, v kotoryh raznymi metodami ocenivaetsya eto rasstoyanie. Povodom dlya rassmatrivaemoi stat'i posluzhila rabota Eizenhauera s soavtorami. Oni geometricheskim metodom (nablyudaya vrashenie zvezd vokrug sverhmassivnoi chernoi dyry) poluchili znachenie 7.94+/-0.42 kpk. V predelah oshibok eto sovmestimo i so standartnym 8.5 kpk i s "korotkim" 7.5 kpk. Novaya ocenka, sdelannaya na osnove monitoringa pul'siruyuzih zvezd, daet znachenie, prakticheski sovpadayushee s privedennym Eizenhauerom i dr.: 7. 94+/-0.37+/-0.26 kpk. Tak chto poka ne poluchaetsya povysit' tochnost'. Navernoe, stoit ispol'zovat' 8 kpk, uchityvaya neopredelennost' v pol-kiloparseka. arxiv:0801.2782 Ukazaniya po dannym Dzhemini i Kosmicheskogo teleskopa im. Habbla na sushestvovanie chernoi dyry promezhutochnoi massy v Omega Centavra (Gemini and Hubble Space Telescope Evidence for an Intermediate Mass Black Hole in omega Centauri) Authors: Eva Noyola, Karl Gebhardt, Marcel Bergmann Comments: 8 pages, 9 figures, ApJ accepted Po dannym opticheskih nablyudenii avtory delayut vyvod o sushestvovanii chernoi dyry promezhutochnoi massy (primerno ot 30 000 do 50 000 mass Solnca) v skoplenii Omega Centavra. V kachestve osnovanii dlya takogo vyvoda avtory ispol'zuyut raspredelenie zvezdnoi plotnosti (oni vidyat harakternyi kasp), a takzhe raspredelenie skorostei (rost dispersii skorostei v centre govorit o koncentracii massy). Obsudit' v ZhZh-soobshestve ru_astroph. Obsudit' na Astroforume v Nauchnoi panorame. obzor arxiv:0801.2944 Fizika vrasheniya v zvezdnyh modelyah (Physics of rotation in stellar models) Authors: Georges Meynet Comments: 32 pages, 7 figures, lectures, CNRS school, will be published by Springer Ochen' horoshie lekcii, posvyashennye razlichnym fizicheskim processam, svyazannym s vrasheniem zvezd, a takzhe ih vliyaniyu na zvezdnye modeli. miniobzor arxiv:0801.2966 Radiotranzienty: sovremennaya i gryadushaya kartiny (Radio Wavelength Transients: Current and Emerging Prospects) Authors: J. Lazio Comments: 4 pages, to appear in proceedings of Hot-wiring the Transient Universe, 2008 March issue of Astronomische Nachrichten Korotkaya zametka, soderzhashaya polnyi spisok horosho ustanovlennyh radiotranzientov, t.e. ob'ektov, dayushih radiovspyshki ili demonstriruyushie sushestvennuyu peremennost' v svoem radioizluchenii. Eto i planety, i Solnce, i burye karliki i t.d. Perechislenie etih ob'ektov s kratkimi harakteristikami zanimaet polovinu nebol'shoi zametki. Vtoraya polovina otvedena pod budushie instrumenty, kotorye v blizhaishie gody zarabotayut i dadut bol'shoi vklad v izuchenie radiotranzientov: ATA, EVLA, LWA, LOFAR, MWA. My budem starat'sya hotya by perechislit' interesnye (dlya shirokoi publiki) stat'i, poyavivshiesya v razdele physics (vklyuchaya cross-listing). arxiv:0801.2700 Etiketki i fizika: razvitie novyh metodov markirovki kak novoe mnogoobeshayushee pole dlya prikladnoi fiziki (Labels discover physics: the development of new labelling methods as a promising research field for applied physics) Authors: Amelia Sparavigna Comments: 16 pages, 9 fihures Chto tol'ko ne ispol'zuyut dlya etiketok i markirovok! A vse dlya togo, chtoby zashitit' tovar ot poddelok ili zhe peredat' informaciyu. Krome uzhe banal'nyh shtrih-kodov i gologramm v etom dele primenyayut dostatochno prodvinutye tehnologii, osnovannye na interesnyh fizicheskih effektah. Koe-chto ob etom mozhno uznat' iz stat'i. Vernut'sya k nachalu stranicy

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