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1. Neutron Star X-ray Binaries with Low-mass Companions
Smithsonian Astrophysical Observatory | Center for Astrophysics | XRB SED Home | . RXTE Light Curves (And tables of SED observation times where available): . 4U0614+091 . 0748-676 (UY Vol) . 1254-69 (GR Mus) . Scorpius X-1 . Hercules X-1/HZ Herculis . Serpens X-1 (MM Ser) . Cyg X-2 . Cen X-4 . J1556-605 . X1603.6+2600 . X1636-53 . X1658-298 . SEDs: . 4U0614+091 . Scorpius X-1 . Hercules X-1/HZ Herculis . Serpens X-1 (MM Ser) . 4U1735-444 . GX9+9 . GX17+2 . GX349+2 . 4U1636-536 . 4U1254-690 . EXO0748-676 .
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~saku/NSXBL.html -- 4.3 Кб -- 01.10.2012
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2. Low-Mass Star Formation
Next: Jets Up: M.D. Smith Previous: High-Mass Star Formation Contents . By contrast, stars of low mass like our Sun are formed within molecular clumps. Michael Smith has been investigating the clumps and the individual cores they contain within one nearby cloud near the star Rho Ophiuchi. With Stanke (Hawaii), Khanzadyan (Heidelberg) and Gredel (Calar Alto), he has determined the masses of over 100 protostellar cores and compared this to the distribution of masses for stars. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/annrep/annrep2004/node58.html -- 5.7 Кб -- 19.04.2005
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3. Galaxy sector, archive 2006
... 2006: . ... Components of the systems are low mass stars and white dwarfs. For 14 pairs orbit parameters were calculated and masses and luminosities of components were determined for the first time. ... As a result of a multifrequency monitoring of the variability of a micro quasar Cyg X-3 (X-ray binary system which probably consists of a black hole and a high mass Wolf-Rayet star) a high activity period was registered for the first time in the last 4 years. ... Archive . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/Science/results/ar_galaxy/res2006.html -- 6.1 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/Doc-en/Science/results/ar_galaxy/res2006.html -- 6.1 Кб -- 10.04.2016
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4. Титарчук Лев Григорьевич (NRL)
... We show the analysis of low-hard and intermediate states of sources XTE J1550-564, H 1743-322, GX 339-4, XTE J1859-226, XTE J1650-500 and GRS 1915+105. ... Directly applying the scaling technique we also obtain that a ratio of the BH masses in XTE J1859-226 and in XTE J1550-564 is , and the corresponding ratio for XTE J1650-500 and XTE J1550-564 is . These values of scaling factors r implies that BH masses are ; solar masses in XTE J1859-226 and XTE J1650-500 respectively. ...
[ Сохраненная копия ]  Ссылки http://hea.iki.rssi.ru/conf/hea2007/abstracts/node70.html -- 6.1 Кб -- 19.12.2007
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5. Астронет > Микролинзирование
... Астронет | ... Переменные Звезды | ... Микролинзирование . ... На протяжении последних нескольких лет в рамках проекта MACHO проводятся наблюдения микролинзирования звезд Большого Магелланова Облака - спутника нашей Галактики. Эффект микролинзирования заключается в гравитационной фокусировке света звезды массивным объектом, находящимся на луче зрения между звездой и наблюдателем. ... Согласно некоторым гипотезам, линзами могут являться реликтовые черные дыры или "нейтралинные звезды". ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/msg/1156993 -- 19.0 Кб -- 31.07.2003
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6. Marat Abubekerov - publications list
... Abubekerov M.K., Lipunov V.M. "The Lower Temperature Limits Of Accretors" Astronomy Reports, 2003, Vol. 47, Issue 8, pp.679-684. ... Abubekerov M.K., Antokhina E.A., Cherepashchuk A.M. "The Masses of X-ray Pulsars in Binary systems with OB Supergiants" Astronomy Reports, 2004, Vol. ... Abubekerov M.K., Antokhina E.A., Cherepashchuk A.M., Shimanskii V.V. "The Mass of the Compact Object in the Low-Mass X-ray Binary 2S 0921-630" Astronomy Reports Astronomy Reports, 2006, Vol.50, Issue 7, pp.544-552. ...
[ Сохраненная копия ]  Ссылки http://lnfm1.sai.msu.ru/~marat/publications.html -- 9.1 Кб -- 12.01.2015
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7. http://www.atnf.csiro.au/research/Astro2008/Postings/George_Hobbs.pdf
From limits to detection of a gravitational wave signal George Hobbs ATNF PPTA team. ... Jenet et al. 2005 Must look for correlated residuals Need ~20 pulsars, observed of ~5 years with rms timing residuals ~100ns Gravitational wave detection Basic ideas Jenet et al. ... 2006 New limit technique (Bill's talk) Improve timing residuals Bayesian Detection technique Gravitational wave detection A Bayesian technique for detecting gravitational waves · Work carried out by Y. Levin and R. van Haasteren. ...
[ Текст ]  Ссылки http://www.atnf.csiro.au/research/Astro2008/Postings/George_Hobbs.pdf -- 1637.5 Кб -- 26.06.2008
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8. What factors determine if a massive star (say, 100 solar masses) forms instead
... Star Atlas . ... solar system . ... stars . ... Observe the Solar System . ... What factors determine if a massive star (say, 100 solar masses) forms instead of a Sun-like star? ... Stars of all masses form from dense clumps within exceptionally cold molecular clouds. ... Massive stars tend to form at the centers of high-mass reservoirs of gas. Get instant access to subscriber content on Astronomy.com! ... A gamma-ray burst hints that LIGO's double black holes started as one massive star . ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/magazine/ask-astro/2012/01/stellar-creation -- 63.1 Кб -- 10.04.2016
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9. http://www.aaa.org/s932/images/09fallclass2.pdf
Class 1 Introduction, Background History of Modern Astronomy The Night Sky, Eclipses and the Seasons Kepler's Laws Newtonian Gravity General Relativity Matter and Light Telescopes Class 2 Solar System Characteristics Formation Exosolar Planets Class 3 Stars The Sun Stellar Evolution of Low and High Mass Stars Deaths of Stars Exotic Stars Class 4 Galaxies Galaxy Classification Formation of Galaxies Galactic Evolution ... So far, one planet has been studied by this method. ...
[ Текст ]  Ссылки http://www.aaa.org/s932/images/09fallclass2.pdf -- 1505.3 Кб -- 07.09.2011
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10. http://www.arcetri.astro.it/~lt/projects/ovro/wams/WamsTalk.pdf
... 1998; Shepherd Kurtz 1998 California Institute of Technology Leonardo Testi Osservatorio Astrofisico di Arcetri Circumstellar disks around TTauri stars Spatially and kinematically resolved gaseous disks around young low mass pre main sequence (TTauri) stars Koerner Sargent California Institute of Technology Leonardo Testi Osservatorio Astrofisico di ...
[ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/projects/ovro/wams/WamsTalk.pdf -- 1689.9 Кб -- 11.09.2007
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11. http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_oct2014/AS01.html
2600) of EBs, roughly 100 of which have been followed up and for which reliable masses, radii, and spectral types have been obtained (Torres et al. 2010). ... To improve constraints on theories of stellar evolution at the low-mass end, we have proposed to use ARCES and DIS (in high-resolution mode) at APO to obtain radial velocity measurements and metallicities for an EB system in the Kepler field containing two K dwarfs. ... REFERENCES: Torres, G., Andersen, J., Gimenez, A. 2010, AAPR, 18, 67 ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_oct2014/AS01.html -- 3.5 Кб -- 08.10.2014
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12. . The . MASS . Group .
... Measurement of the MASS detectors parameters with mass program January 24, 2015 [112707] . MASS/DIMM electronics. ... Turbina-core(D): Dimm User Guide. ... N.Shatsky, V.Kornilov, The revision of the MASS/DIMM star catalogue. ... О.Возякова, В.Корнилов, Н.Шатский, Новое программное обеспечение прибора MASS/DIMM. ... V.Kornilov, N.Shatsky, S.Potanin, O.Voziakova, B.Safonov Preliminary results of astroclimate parameters measurements at the Sternberg 2.5m telescope installation site. ...
[ Сохраненная копия ]  Ссылки http://curl.sai.msu.ru/mass/docs.shtml -- 10.3 Кб -- 27.06.2015
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13. Rest Mass - an Astronomy Net Blackholes Forum Message
Blackholes Forum Message . ... Post . ... Rest Mass . ... Post Message | ... When the atom was first measured it was assumed to be composed of rest mass. ... The mass due to motion with respect to an observer approaches 0 as the velocity approaches 0. ... If a photon has a zero rest mass and therefore is composed entirely of momentum mass. ... www.astronomy.net . ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.net/forums/blackholes/messages/6598.shtml -- 14.2 Кб -- 09.04.2016
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14. Rambler Mass Media
... 30-10-2003 10:37 Rambler Mass Media . Японские ученые утверждают, что обнаружили воду на крупном астероиде (малой планете) Веста, который движется между орбитами Марса и Юпитера. ... Планета вращается вокруг неподвижной .. ... Космический зонд "Галилео" завершил свою миссию . ... NASA испарит спутник Galileo в атмосфере Юпитера . ... Американское аэрокосмическое агентство NASA планирует в конце сентября распылить спутник Galileo стоимостью 1,5 млрд долл. в атмосфере Юпитера. ...
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/events/from/rambler.html?page=4 -- 14.1 Кб -- 11.04.2016
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15. http://mavr.sao.ru/hq/katya/CosmosPh/en/Abstract_Sharina.txt
Results from 6m telescope observations of globular clusters in dwarf galaxies Sharina M. We consider properties of globular clusters in dwarf galaxies observed with the multi-slit unit of the SCORPIO spectrograph at the SAO 6m telescope. ... Studying GCs in dwarf galaxies at the faintest end of the galaxy luminosity function provides valuable information for a better understanding of galaxy evolution and evolutionary connection between globular clusters and nuclei of galaxies. ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/katya/CosmosPh/en/Abstract_Sharina.txt -- 2.3 Кб -- 16.05.2007
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/katya/CosmosPh/en/Abstract_Sharina.txt -- 2.3 Кб -- 24.02.2010
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/katya/CosmosPh/en/Abstract_Sharina.txt -- 2.3 Кб -- 24.02.2010
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16. HIGH RESOLUTION IONOSPHERIC MASS SPECTROMETER P-11
HIGH RESOLUTION IONOSPHERIC MASS SPECTROMETER P-11 . ... Onboard mass-spectrometric equipment for study of neutral and ionized components of Earth upper atmosphere. Mass-spectrometer P-11 is one of P-series modifications of the on board radio-frequency monopole spectrometers. ... The instruments of P-series have passed successful approbation in space experiments aboard geophysical rockets MP-12, launched for investigation of Earth upper atmosphere (Ref. ... Measured mass number range, AMU - 1.. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/projects/warning/p-11.html -- 5.7 Кб -- 15.02.2000
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17. Igor Antokhin
. To see a Russian version of this page click here . (Senior Researcher. Graduated from Moscow State University (MSU) in 1982, Ph.D. 1986, MSU) . A member of EAS and IAU. Fields of interest: hot massive stars, close binary systems: optical photometric and spectral observations, X-ray observations; ill-posed problems, X-ray astrophysics. My publications (ADS link) . Linux on CLEVO 8750 (old stuff) . Phones/addresses of my university mates graduated in 1982. E-mail: igor@sai.msu.ru .
[ Сохраненная копия ]  Ссылки http://uranus.sai.msu.ru/~igor/ -- 3.5 Кб -- 01.07.2010
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18. ASP: Black Holes to Blackboards: The Sun is a Mass of Incandescent Gas
... Not only can the Sun turn night to day, it can transform obscure 1950s jingles into 1990s alternative-rock hits. ... The sun is a mass of incandescent gas, . ... Studying the Sun can tie together subjects across the curriculum. ... Sunspots and prominences--the tongues of hot plasma which shoot off the Sun's surface and arch gracefully back, following the invisible tethers of magnetic field lines--are just two examples of solar volatility. ... The black dots will be easy to see. ...
[ Сохраненная копия ]  Ссылки http://www.astrosociety.org/pubs/mercury/9705/lockwood.html -- 12.1 Кб -- 02.10.2012
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19. http://site2010.sai.msu.ru/static/doc/BSafonov_site2010.pdf
Twilight observations with MASS/DIMM B. Safonov Sternberg Astronomical Institute Moscow State University Comprehensive Characterization of Astronomical Sites, 2010 B. Safonov (Moscow State University) Twilight observations with MASS/DIMM SITE 2010 1 / 17 Why observe in twilight with MASS/DIMM? ... ASM includes 3 devices sensitive to background: guider, DIMM and MASS. B. Safonov (Moscow State University) Twilight observations with MASS/DIMM SITE 2010 2 / 17 Background in guider. ...
[ Текст ]  Ссылки http://site2010.sai.msu.ru/static/doc/BSafonov_site2010.pdf -- 705.7 Кб -- 18.10.2010
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20. Globular clusters with anomalously small masses, figures
... The relationship of the mass and the observed galactocentric distance R -- (a), and that of the mass and the total dissipation velocity n taken from Gnedin, Ostriker (1997) -- (b). The dotted line in diagram (a) shows the "cone of survival" according to the paper by Surdin and Arkhipova (1998) . ... The solid line is a regression stright line for the main sequence of clusters, and the dotted line parallel to it separates the sequence of clusters of anomalously small mass shown by open triangles. ...
[ Сохраненная копия ]  Ссылки http://ip.rsu.ru/~marsakov/paper8/p8fg1_1.htm -- 2.9 Кб -- 02.02.2007
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