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http://www.astronet.ru/db/varstars/msg/1273942.
http://www.astronet.ru/db/varstars/msg/1273942.
1. Journal "Peremennye Zvezdy"
Peremennye Zvezdy", . ... Period . ... Comment . ... see Comments) . ... Comments: . ... The variable is listed in the GCVS as an RR star without light elements. V0722 Cen has been identified as a double-mode RR Lyrae star, type RR(B), by analysis of Catalina Real-Time Transient Survey (CRTS) data (Drake et al. ... The light elements are: . ... It is listed in the GCVS as an RR: star without light elements, with a reference to Bond (1978). ... The period is unusually long period for this type. ...
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Ссылки http://www.astronet.ru/db/varstars/msg/1283540 -- 22.8 Кб -- 08.01.1973
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2. Supernova 2009js in NGC 918
Supernova 2009js in NGC 918 . This page is devoted to information on Supernova 2009js in NGC 918 . Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . Information on the original web pages for many of these images can be found on the updates and links web pages. Discovered independently by Lick Observatory Supernova Search (USA) and Koichi Itagaki (Japan). ... 2009/10/11.44 . 17.2 . ... Joseph Brimacombe . ...
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Ссылки http://www.sai.msu.su/mirrors/isn/sn2009/sn2009js.html -- 8.2 Кб -- 13.02.2011
[ Сохраненная копия ] Ссылки http://www.rochesterastronomy.org/sn2009/sn2009js.html -- 8.4 Кб -- 19.04.2014
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[ Сохраненная копия ] Ссылки http://www.rochesterastronomy.org/sn2009/sn2009js.html -- 8.4 Кб -- 19.04.2014
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3. Examples of GHRS Phase II Proposals
Your Phase II Proposal and Using RPS2 . ... Exposure_Number: 1 Target_Name: HD12345 Config: HRS Opmode: ACQ Aperture: 2.0 Sp_Element: MIRROR-N1 Wavelength: Optional_Parameters: BRIGHT=RETURN, ! ... Number_of_Iterations: 1 Time_Per_Exposure: 13.5S Special_Requirements: ONBOARD ACQ FOR 2 Comments: STEP-TIME = 1.5 sec Exposure_Number: 2 Target_Name: HD12345 Config: HRS Opmode: ACQ/PEAKUP Aperture: 0.25 Sp_Element: MIRROR-N1 Wavelength: Optional_Parameters: SEARCH-SIZE=5 ! ...
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Ссылки http://www.stsci.edu/instrument-news/handbooks/ghrs/GHRS_24.html -- 10.9 Кб -- 14.02.1996
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4. The AstroStat Slog data mining
... Posts tagged ?data mining? ... Posted by hlee . ... Book] The Elements of Statistical Learning, 2nd Ed.? Tags: book , Brieman , cigar , Clinton , data mining , Friedman , Hastie , KDD , light curve , machine learning , SCMA , shaking hands , SN , statistical learning , Supernova , Tibshirani . ... Thanks to a Korean solar physicist [ 1 ] I was able to gather the following websites and some relevant information on Space Weather Forecast in action, not limited to literature nor toy data. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/tag/data-mining/index.html -- 34.5 Кб -- 01.03.2014
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5. First X-Rays From a Comet Discovered
A team of U.S. and German astrophysicists have made the first ever detection of X-rays coming from a comet. ... Following the initial detection, the team reported repeated X-ray emissions from the comet over the next 24 hours. ... One preliminary theory is that X-ray emission from the Sun was absorbed by a cloud of gaseous water molecules surrounding the nucleus of the comet, and then were re-emitted by the molecules in a process physicists call "fluorescence." ... Comets . ...
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Ссылки http://www.iki.rssi.ru/solar/eng/hyakutak.htm -- 5.3 Кб -- 15.10.1997
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6. (Untitled)
... They were determined as a result of orbit improving on the base of all kinds of optical observations available in the catalog of observations of the Minor Planet Center on March 16, 2014 (radar observations have not been used at this stage). ... As the MPC orbits do not all were improved simultaneously with EMP orbits, only 383866 sets of elements were used for data comparison (for selected sets of elements process of improvement had started with the use of the same observations). ...
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Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user4dpi.htm -- 12.5 Кб -- 10.04.2016
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7. Exoplanet HAT-P-1b: weird, warm and fuzzy | Astronotes
... Planets . ... Stars . Exoplanets . ... Most exoplanets so far discovered fall into the category of тАШhot JupitersтАЩ, these are giant planets orbiting very close to their parent star. ... Note that we have discovered so many hot Jupiters because they are the easiest type of planet to find, they are not necessarily particularly common in the galaxy. ... Subsequently several similar hot and€а fuzzy worlds have been discovered the same way, proving this that this planet is not a one-off oddball. ...
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Ссылки http://www.armaghplanet.com/blog/exoplanet-hat-p-1b-weird-warm-and-fuzzy.html -- 43.8 Кб -- 09.04.2016
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8. Package: dmp
... dmp_multi_desc . Dump a multi_array descriptor to a file. dmp_packet_desc . Dump a packet descriptor to a file. dmp_element_desc . Dump an element descriptor to a file. dmp_array_desc . ... Dump a linked list to a file. dmp_flag . Dump a flag value to a file. void dmp_multi_desc (FILE *fp, multi_array *multi_desc, flag comments) . ... fp : The file pointer. multi_desc : The descriptor. comments : If TRUE, the routine will append comments to the lines written, else it will not. ...
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Ссылки http://www.atnf.csiro.au/computing/software/karma/lib/dmp.html -- 9.2 Кб -- 24.12.2007
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9. RadioAstron Mission Element Overview
Next: RSOG Pre-Observation Products . ... Mission Elements . ... The main mission elements (ME) are: . The RSOG, based at ASC, which is responsible for the science operation of the RadioAstron Mission. ... The Main Ballistic(Navigation) Center (MBC) belonging to Lavochkin Association coordinates preparation and exchange of orbit determination and orbit reconstraction ptoducts. ... Experiment codes of five characters are used in naming GRT related files. ... RSOG . ... Corr (GTS?) ... Corr (RSOG?) ...
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Ссылки http://www.asc.rssi.ru/RadioAstron/documents/rmoh/eng/rameo.htm -- 14.7 Кб -- 30.08.2001
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10. http://www.astro.louisville.edu/shared_skies/archive/select/comets/ison/20120929/ison.txt
From XEphem running the Soft03Cmt database of 20121002, for the date and time of the observation: RA: 08:16:04.25 Dec: 27:48:13 2012-09-30 UT 09:45 UTC Measured: RA: 08:16:04.4 Dec: 27:48:12.9 Header listing for HDU #1: SIMPLE = T / This is a FITS file BITPIX = -32 / NAXIS = 2 / NAXIS1 = 4341 / NUMBER OF ELEMENTS ALONG THIS AXIS NAXIS2 = 4355 / NUMBER OF ELEMENTS ALONG THIS AXIS EXTEND = T / This file may contain ...
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Ссылки http://www.astro.louisville.edu/shared_skies/archive/select/comets/ison/20120929/ison.txt -- 4.8 Кб -- 02.10.2012
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11. http://www.arcetri.astro.it/irlab/luna/firpo/firpo_publ.html
Last modified on August 19, 1996 by A. Richichi . ... Hamilton, D.P., Herbst, T.M., Richichi, A., B?hnhardt, H., Ortiz, J.L. 1995, '' Calar Alto observations of Shoemaker-Levy 9: characteristics of the H and L impacts '', Geophysical Research Letters, 22 , 2417. ... Hamilton, D. P., Herbst, T. M., B?hnhardt, H., Ortiz-Moreno, J. L., Richichi, A., Calamai, G. 1995, `` Calar Alto Observations of the A, H, L, Q1 and Q2 Impacts '', Proceedings of the XXIInd General Assembly of the IAU, den Haag 15-27 Aug. ...
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Ссылки http://www.arcetri.astro.it/irlab/luna/firpo/firpo_publ.html -- 4.8 Кб -- 28.07.2005
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12. APOD: 2001 October 26 - Elements in the Aftermath
... 2001 October 26 . Elements in the Aftermath . ... CXC , NASA . ... And so a supernova explosion , a massive star's inevitable and spectacular demise, blasts back into space debris enriched in heavier elements to be incorporated into other stars and planets (and people! ... Just below and left of center, a point like object in the Chandra image suggests that the enriching supernova also produced a pulsar in its aftermath, a rotating neutron star remnant of the collapsed stellar core. ...
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Ссылки http://www.sai.msu.su/apod/ap011026.html -- 5.3 Кб -- 01.10.2012
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13. Comet Ephemerides
... To save time, I will only provide ephemerides in 2000 coordinates. ... Note: most the orbital elements used to create these ephemerides were obtained from the International Astronomical Union Circulars (IAUCs), Minor Planet Circulars (MPCs) or the ICQ Comet Handbook. ... The following 1-day ephemeris (March 1, 1997 - October 1, 1997) is from Donald Yeomans of JPL and is based on Reference Orbit #55 (March 4, 1997). 2000 coordinates (March - September, 1997) [3/4/97] . ... Epoch: 1997 Feb. 1.0 . ...
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Ссылки http://www.issp.ac.ru/univer/astro/comets/eph.html -- 6.3 Кб -- 11.04.2001
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14. Amateur Telescope Makers of Boston
... Submitted by Al Takeda on 09/24/2015 13:03:02 . Veil Nebula - Supernova Remnant . The Veil Nebula is a supernova remnant located in the Cygnus constellation. ... The entire Veil Nebula covers an area more than 3 degrees, which is 6 times the diameter of the full moon. ... AstroTech AT66, 66mm, f/5 ED Refractor using an AstroTech flat field corrector, SBIG STL-6303E monochrome CCD camera, Losmandy Gemini G-11 EQ mount. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...
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Ссылки http://www.atmob.org/gallery/showimage.php?id=3037 -- 3.9 Кб -- 10.04.2016
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15. Comments
... Rounds up rebinned pixel size to the nearest integer multiple of the elementary size of the input image . Ignores pixels on the edges that do not fit in an integer number of rebinned pixels . The ancilliary response file for the output spectra should be created with SAS task arfgen . When dealing with filter masks, arfgen works by averaging the ARF in a number of grid elements on an internal map, thus, it is necessary to allow a large number of elements in the internal arfgen map: . ...
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Ссылки http://xmm.vilspa.esa.es/sas/7.1.0/doc/flspec/node9.html -- 4.2 Кб -- 09.07.2007
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16. Rivi: Be Stars
... Be Stars . ... Stellar Winds . ... He had found the first emission line star. ... More emission line stars were found soon, and one had to make subclasses to keep some overview. Cas is a main sequence B-type star, and together with other such stars showing hydrogen emission it forms the class of "Be stars", where the "e" stands for emission. ... Struve further speculated that those stars would be surrounded by a disk, basically thrown off the stellar surface by the rapid rotation. ...
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Ссылки http://www.eso.org/~triviniu/be.php -- 6.5 Кб -- 01.10.2012
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17. Supernova light echoes discovered | Astronomy.com
... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... Supernova light echoes discovered . ... R ecently discovered light echoes can be traced back to three ancient supernova remnants in the Large Magellanic Cloud (LMC), say astronomers. ... Astronomers performed an image analysis on their survey data and matched the discovered light echoes to three young LMC supernova remnants. ... Only registered members of Astronomy.com are allowed to comment on this article. ...
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Ссылки http://www.astronomy.com/news/2006/01/supernova-light-echoes-discovered -- 69.1 Кб -- 10.04.2016
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18. Understanding HTML and SGML
HTML is an application conforming to International Standard ISO 8879 -- Standard Generalized Markup Language (SGML). ... Every SGML document has three parts: . SGML declaration . ... For example, the SGML declaration in the HTML DTD specifies that the string that opens an end tag is </ and the maximum length of a name is 72 characters. ... Most HTML elements are identified in a document as a start tag, which gives the element name and attributes, followed by the content, followed by the end tag. ...
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Ссылки http://comet.sai.msu.ru/webdesign/html-3.0/HTMLandSGML.html -- 9.5 Кб -- 19.12.1996
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19. source comment
. Comment on J0318+4151 . No detection: according to global VLBI observations at 5 GHz by Xu, O'Dea & Biretta (1999), the core of this double-tail radio galaxy has a brightness of 13 mJy/beam, too weak for us to be detected. VLBApls home page . Last modified: 16 Oct 2000
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Ссылки http://www.vsop.isas.ac.jp/VLBApls/J0318+4151.comment.htm -- 1.5 Кб -- 16.10.2000
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20. Physicists from Samara and Novosibirsk discovered a new phenomenon
... Scientists from G. I. Budker Institute of Nuclear Physics- Syberian Branch of the Russian Academy of Science, Novosibirsk State University, Novosibirsk State Technical University, Samara State Aerospace University (SSAU) and Image Processing Systems Institute (IPSI) of the Russian Academy of Science, became the first people in the world obtained terahertz non-diffractive twisted Bessel beams and used them for the first time the formation of surface electromagnetic waves on the metal surface. ...
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Ссылки http://www.ssau.ru/engnews/11891/ -- 26.2 Кб -- 23.10.2015
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