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http://hea-www.harvard.edu/~garcia/m31/garcia_chandra6y_short.pdf.
http://hea-www.harvard.edu/~garcia/m31/garcia_chandra6y_short.pdf.
1. Kinematics of galaxies: catalogue
. Back to A.Zasov's homepage.
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Ссылки http://neptun.sai.msu.su/~zasov/menucat.html -- 1.7 Кб -- 15.01.1999
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2. *qpspec* - Time Resolved Spectral Fitting
... xs qpspec source qpoe file (xdata$rp110590n00.qp): xdata$rp110590n00.qp[ time =(1606720.00:1607479.00)] source region descriptor ():c 6947 9325 2' background qpoe file ( ): bkgd region descriptor (): a 6947 9325 3' 4' root name for output files [root_obs.tab, etc.] (): arlac_1 ds: 0 file : arlac_1_obs.tab scale: 0.00 mission: 20 seqno: CA110590P.N6 instrument: ROSAT_PSPC sub-instrument: 1 no. pha channels: 34 mean off-axis angle of events (arcmin ...
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Ссылки http://hea-www.harvard.edu/PROS/PUG/node162.html -- 6.1 Кб -- 01.10.2012
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3. A Panchromatic View of NGC 602: Time-resolved Star Formation with the Hubble
We present the photometric catalogs for the star-forming cluster NGC 602 in the wing of the Small Magellanic Cloud covering a range of wavelengths from optical (HST/ACS F555W, F814W, and SMARTS/ANDICAM V, I) to infrared (Spitzer/IRAC 3.6, 4.5, 5.8, and 8 ЮМm and MIPS 24 ЮМm). ... We demonstrate a progression of star formation from the optical star cluster center to the edge of the star-forming dust cloud. ...
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Ссылки http://www.stsci.edu/~kgordon/papers/2011ApJ...730...78C.html -- 4.9 Кб -- 21.01.2016
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4. ESO - RASPUTIN: Resolved And unresolved Stellar PopUlaTIoNs
... Science . ... Science Users Information > Science Publications > Science Announcements > RASPUTIN: Resolved And unresolved Stellar PopUlaTIoNs . ... During the workshop the impact that the European Extremely Large Telescope (E-ELT) and its first generation instruments will have on resolved and unresolved stellar population studies will be discussed. Registration is open until 12 September 2014 and further information is available from the RASPUTIN webpage or by email to: rasputin@eso.org . ...
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Ссылки http://www.eso.org/sci/publications/announcements/sciann14010.html -- 23.5 Кб -- 10.04.2016
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5. HyperLEDA documentation: Resolved Kinematics
Catalogue of Spatially Resolved Kinematics of galaxies . ... The goal of the present project is to built a catalogue gathering references to all spatially resolved studies, for galaxies of all types, whatever the gas or stellar content is concerned. The catalogue has been assembled from merging the lists of Corradi and Capaccioli (1990) and Prugniel and Simien (1996). ... In total, the published catalogue contains 4165 observations of 2070 galaxies referring to 743 published papers. ...
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Ссылки http://www.sao.ru/fetch/HL/05/ -- 4.7 Кб -- 23.12.2013
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6. Optical Transient Near GRB970508 Shows Distant Redshift
... U. Amsterdam Explanation: The GRB distance scale controversy may have just ended with a flash . Gamma Ray Bursts (GRBs) are powerful explosions occurring in seemingly random positions on the sky. ... There they found a faint but variable optical source : a potential counterpart to the gamma-ray burst that was getting brighter. Most importantly, continued scrutiny showed that this optical transient had absorption lines with a redshift of about 0.8 - the distance scale of galaxies and quasars . ...
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Ссылки http://www.astronet.ru/db/xware/msg/apod/1997-05-13 -- 14.8 Кб -- 23.06.2003
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7. APOD: May 13, 1997 - Optical Transient Near GRB970508 Shows Distant Redshift
... May 13, 1997 . Optical Transient Near GRB970508 Shows Distant Redshift . ... Explanation: The GRB distance scale controversy may have just ended with a flash . ... Most importantly, continued scrutiny showed that this optical transient had absorption lines with a redshift of about 0.8 - the distance scale of galaxies and quasars . ... Above is a "negative" image of the GRB970508 field , located near the north celestial pole, taken hours after the initial flash of gamma rays. ... About APOD > . ...
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Ссылки http://www.sai.msu.su/apod/ap970513.html -- 5.1 Кб -- 02.10.2012
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8. http://www.mso.anu.edu.au/seminars/abstracts/20150206-1400.html
Our understanding of star formation in galaxies is facilitated by observations, at multiple wavelengths, of emission which traces stellar populations. ... Using optical integral field spectroscopy, my work aims to better understand the local SFR calibrations, which use H-alpha and radio continuum emission, when applied to different regions of a galaxy, as well as to galaxies as a whole. ...
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150206-1400.html -- 4.8 Кб -- 10.04.2016
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9. Armagh Observatory Preprint No. ???
... A series of 59 moderate-resolution high signal-to-noise spectra of the pulsating helium star V652 Her covering 1.06 pulsation cycles was obtained with the William Herschel Telescope. ... self-consistent high-precision measurements of effective temperature and surface gravity around the pulsation cycle, . ... Keywords: stars: fundamental parameters -- stars: abundances -- stars: helium -- stars: individual (V652 Her) -- stars: pulsation -- techniques: spectroscopic . ...
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Ссылки http://star.arm.ac.uk/~csj/papers/abstracts/v652her5.html -- 4.4 Кб -- 01.07.2002
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10. Holeum - Black Matter Mystery Resolved? - an Astronomy Net Blackholes2 Forum
Blackholes2 Forum Message . Forums: . Atm ћ Astrophotography ћ Blackholes ћ Blackholes2 ћ CCD ћ Celestron ћ Domes ћ Education . ... Discussion Forums | ... Holeum - Black Matter Mystery Resolved? Forum List | ... Post Message | ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
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Ссылки http://www.astronomy.net/forums/blackholes2/messages/4871.shtml -- 16.4 Кб -- 09.04.2016
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11. G67.8+0.5
. Right Ascension: 20 00 00 . Declination: +30 51 . Size (/arcmin): 7?5 . Type: ? . Flux density at 1 GHz (/Jy): ? . Spectral Index: ? . Radio: Poorly resolved arc. Optical: Diffuse shell, brighter to W. References: . Sabin et al. 2013, MNRAS, 431, 279. H and radio survey observations. ADS . Last updated: 30 Apr 2014 . home | documentation | detailed listings | summary listings . Dave Green/Cambridge, UK/ D.A.Green@mrao.cam.ac.uk
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Ссылки http://www.mrao.cam.ac.uk/projects/surveys/snrs/snrs.G67.8+0.5.html -- 2.6 Кб -- 10.04.2016
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12. ATNF Daily Astronomy Picture
16th of June 2015 . ASKAP HI imaging of the galaxy group IC 1459 . ... One of these observations was aimed at studying the distribution of neutral hydrogen (HI) gas in the galaxy group IC 1459. ... HI found outside galaxies in this group amounts to at least 10% of the HI contained inside galaxies. This suggests a substantial flow of gas in and out of galaxies during the several billion years of the group's evolution. ... today * ATNF | ... ASKAP | ...
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Ссылки http://www.atnf.csiro.au/ATNF-DailyImage/archive/2015/16-Jun-2015.html -- 4.9 Кб -- 10.04.2016
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13. XMM Deep Survey Simulations
... QSO spectra in the ROSAT band are steeper than the background at harder energies, and furthermore at fluxes below 1E-14 ergs/(s cmќ) the quasar source counts flatten off and are replaced by more numerous populations of relatively low red-shift objects, apparently Narrow Emission Line Galaxies (NELG). ... We extracted the luminosity function from ROSAT Deep Survey results, and extrapolated by a factor of 2 - 3 to account for changes expected in the harder XMM band. ...
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Ссылки http://xmm.vilspa.esa.es/user/sciobj/deep_survey.html -- 6.2 Кб -- 24.02.1998
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14. APOD: 2001 January 21 - Resolving Mira
... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2001 January 21 . Resolving Mira . ... FOC , ESA , NASA . Explanation: Most stars appear only as points of light. ... Mira was discovered to be the first variable star about 400 years ago by David Fabricus. ... Possible explanations include gravitational perturbation and/or heating from Mira's white dwarf star companion. ... About APOD | ...
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Ссылки http://www.sai.msu.su/apod/ap010121.html -- 4.7 Кб -- 01.10.2012
[ Сохраненная копия ] Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Stelle/mira_hst.htm -- 4.6 Кб -- 22.01.2001
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[ Сохраненная копия ] Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Stelle/mira_hst.htm -- 4.6 Кб -- 22.01.2001
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15. Astro-2 and the UIT Experiment
We report here on those proposed UIT targets that, in fact, were successfully acquired. ... Note on Filters: . A1 centered at 2500 angstroms with a width of 1200 angstroms . ... Sextans A is a low mass dwarf companion to the Milky Way Galaxy. It is sufficiently close that it is easily resolved into its individual stars. ... An exposure of 1100 seconds through the A1 and B1 filters was obtained. NGC 2903 Is a relatively nearby mostly face-on galaxy with active star formation. ...
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Ссылки http://zebu.uoregon.edu/uit-t4.html -- 3.5 Кб -- 07.10.1996
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16. http://www.naic.edu/vscience/schedule/tpfiles/BhattagP1426tp.ps
P1426 2000-Jun-01 22:34:47 Technical Page Proposal Type: Regular General Category : Pulsars Observation Category : Galactic Total Time Requested: 30 Hours Proposal Title: Pulsar Phase-resolved Spectra at High Frequencies: Investigation of the Radio Emission Mechanism ABSTRACT: The proposed work involves a systematic study of pulsar phase-resolved spectra at high frequency bands of ... We will observe several nearby pulsars at 1.2{1.7 GHz, 2{3 GHz and 4{6 GHz bands. ...
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Ссылки http://www.naic.edu/vscience/schedule/tpfiles/BhattagP1426tp.ps -- 96.6 Кб -- 19.04.2004
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17. IV International Astronomy Olympiad, Problems to solve
IV International Astronomy Olympiad . ... Text of these problems is available also . ... To solve every problem you may use constants and well-known values you know by heart. ... The apparent diameter of the Moon, as seen from the Earth, is 31'. ... Can you observe a star with magnitude . ... Consider the stars as black bodies. ... Estimate the diameter of a black hole constructed using this patent from a ship with the mass of 5000 tn (1 tn = 1000 kg). ... What stars would you observe this nigth? ...
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Ссылки http://www.issp.ac.ru/iao/1999/problems/vi99us_e.html -- 11.5 Кб -- 15.04.2011
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18. http://www.astro.spbu.ru/staff/ilin2/INTAS/P3-SPB1/PUBL/ABSTR/fi-mst.txt
On checking the calculations of the optical properties of non-spherical particles V G Farafonov^1 and V B Il'in^2 ^1 St.Petersburg University of Aerocosmic Instrumentation, Bol.Morskaya ul. ... 2, St.Petersburg 198504, Russia Abstract All mathematical and computational problems of the light scattering theory for spherical particles (Mie theory) are well studied and resolved. ... The reciprocity relation is shown to be a useful test (under some conditions), specifically for absorbing scatterers. ...
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Ссылки http://www.astro.spbu.ru/staff/ilin2/INTAS/P3-SPB1/PUBL/ABSTR/fi-mst.txt -- 2.6 Кб -- 19.11.2010
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19. Practical Astrophysics
Subject, Object and Problems of Astrophysics. Practical and Theoretical Astrophysics. ... Visual Telescope; Problems Which Are Solved with the Its Help. ... Resolution of Telescopes. ... Effectiveness of Telescope in Respect of Resolution. ... Optical Power of Telescopes for Star-like and Extensive Objects. Boundary Magnitude. Reasons of Light Dissipation in Telescopes. ... Spectral Instruments in Astrophysics. ... Basic Photometrical Ideas, Magnitudes and Their Measurement. ...
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Ссылки http://space.univ.kiev.ua/courses/pract_astroph_e.html -- 7.6 Кб -- 23.02.2005
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20. MS Windows Netscape 3.0b4 KeepAlive problem solved
Date: Mon, 1 Jul 1996 16:03:06 -0700 (PDT) From: Alexei Kosut <akosut@organic.com> To: Apache Group Subject: Re: keepalive and windoze Good news and good news (of a sort).. I was able to snag a Windows 95 machine here at Organic, and tried out some things: 1) On Netscape 3.0b4, I was able to reproduce the bug, each and every time. ... Alexei Kosut <akosut@organic.com> The Apache HTTP Server http://www.nueva.pvt.k12.ca.us/~akosut/ http://www.apache.org/ . ...
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Ссылки http://neptun.sai.msu.su/manual/misc/windoz_keepalive.html -- 3.3 Кб -- 15.10.2001
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