1. Nebulae in Aurigae
... Nebulae in Aurigae . ... Credit Copyright: Fritz Helmut Hemmerich Explanation: Rich in star clusters and nebulae, the ancient constellation of the Charioteer (Auriga) rides high in northern winter night skies. ... Also known as the Flaming Star Nebula , its red, convoluted clouds of glowing hydrogen gas are energized by hot O-type star AE Aurigae . ... IC 417 and NGC 1931 at the lower right, the Spider and the Fly , are also young star clusters embedded in natal clouds that lie far beyond IC 405. ...
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http://www.astronet.ru/db/xware/msg/apod/2015-12-01 -- 15.1 -- 01.12.2015
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2. APOD: 2015 December 1 - Nebulae in Auriga
... 2015 December 1 . Nebulae in Auriga . ... Explanation: Rich in star clusters and nebulae, the ancient constellation of the Charioteer ( Auriga ) rides high in northern winter night skies. ... Also known as the Flaming Star Nebula , its red, convoluted clouds of glowing hydrogen gas are energized by hot O-type star AE Aurigae . ... The star forming region is famous for its embedded young star cluster, NGC 1893 , and tadpole-shaped clouds of dust and gas. ... About APOD | ...
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http://www.sai.msu.su/apod/ap151201.html -- 5.9 -- 10.04.2016
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3. Arcetri Star-Formation Group Publications
... 2000, ApJ, 537, L49 . ... F. Palla . Invited Talk at the IAU Symposium 200 "The formation of binary stars" eds. R.D. Mathieu and H. Zinnecker (ASP Conf. Ser.) in press . Optical follow-up of ROSAT discovered candidate members of the open cluster Coma Berenices . ... 2000, A , in press . ... 2000, ApJ, in press . ... 2000, ApJ, in press (Sept. ... 2000, ApJ Lett., in press . ... Click to examine publications from other years . ... Star Formation Group . ... Arcetri Home Page . ...
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http://www.arcetri.astro.it/science/starform/publ2000.htm -- 12.8 -- 21.06.2001
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4. Dusty HII Regions and Planetary Nebulae
There is often dust associated with ionized regions. Compact HII regions usually have associated dust from a molecular cloud in which the massive star is being "born". ... For such stars the dust is not produced by the star, and a variety of dust features are observed. The planetary nebulae also usually have associated dust from the previous stage of evolution where they were either carbon stars or M-type giants. ... The feature near 11.5 microns in the IC 418 spectrum may be due to SiC dust. ...
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http://www.stsci.edu/~volk/features3.html -- 6.2 -- 27.05.2014
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5. http://www.mso.anu.edu.au/~bessell/thumbnails/images.txt
GALAXIES cenA .tiff 40 Bright Radio Galaxy M31.tiff Nikon Andromeda Galaxy (note HII regions in spiral arms) ngc6744.tiff 40 NGC 6744 a face-on spiral clouds_20d.tiff H'blad The Magellanic Clouds our nearest neighbours Lmc_7.tiff Nikon The Large Magellanic Clouds Lmc_zoom.tiff Nikon Detail of previous image smc_7.tiff Nikon The Small Magellanic Clouds smc-zoom.tiff Nikon Detail of previous image 30dor_40_BVR.tiff 40 The 30 Dor ... B [OIII] Halpha trifid.tiff 40" The Trifid Nebula. ...
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http://www.mso.anu.edu.au/~bessell/thumbnails/images.txt -- 8.7 -- 27.01.2004
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6. Amateur Telescope Makers of Boston
... Tadpole Emission Nebula and the Flaming Star Nebula . The constellation of Auriga harbors the cluster NGC 1893 which contains the Tadpole Nebula (IC 410). ... The Flaming Star Nebula, IC 405, is the magenta/purplish area and is the reflection portion of this nebulous region. 5nm Narrowband filters; H-alpha: O-III: S-II - 60: 60: 40 minutes x 600-second sub frames, Total= 2-hours 40-minutes, binned 1x1. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...
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http://www.atmob.org/gallery/showimage.php?id=1981 -- 4.0 -- 10.04.2016
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7. A Spectacular View of the Lagoon Nebula | Astronotes
Astronotes Armagh Planetarium's Stellar Blog! ... Stars . ... Telescopes and Observatories . ... The majestic star-forming region in the Lagoon Nebula. The pale ring to the right is an internal reflection in the telescope. (Image credit: ESO/ VPHAS+/ V. Kalari and J. Vink (Armagh Observatory) . ... The 18 component images were further processed twice. ... Venu and his colleagues use images like this to identify individual young forming stars in the Lagoon Nebula and determine their ages. ...
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http://www.armaghplanet.com/blog/a-spectacular-view-of-the-lagoon-nebula.html -- 45.4 -- 09.04.2016
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8. AdelePlunkettAstro
... PhD Yale University, Astronomy, 2015 . ... MS, MPhil Yale University, Astronomy, 2011 . ... Plunkett, Adele L. ; Arce, Hctor G.; Corder, Stuartt A.; Dunham, Michael M.; Mardones, Diego; Garay, Guido 2014, ApJ, 803, 22, Assessing molecular outflows and turbulence in the protostellar cluster Serpens South . ... Department of Astronomy Seminar, Universidad de Chile, Santiago, Chile April 2013 . ... Yale-University of Chile Meeting, New Haven, CT December 2011 . ...
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http://www.eso.org/~aplunket/cv.html -- 10.7 -- 15.01.2016
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9. SAI OCL Catalog Publications
... Catalog . Publications . ... Koposov, S., Glushkova, E., Zolotukhin, I. 2008: Automated search for Galactic star clusters in large multiband surveys. ... BibTeX entry ] . ... Glushkova, E.V., Zabolotskikh, M.V., Koposov, S.E., Spiridonova, O.I, Vlasyuk, V.V., Rastorguev, A. S. 2010: Photometry of the poorly studied galactic open star clusters King 13, King 18, King 19, King 20, NGC 136, and NGC 7245 , Astronomy Letters, 36, 75 . ...
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http://ocl.sai.msu.ru/publications/ -- 5.7 -- 09.04.2016
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10. SCORPIO: IFP Gallery
IFP gallery SCORPIO (since 2000). Here some data observed on the 6m telescope with IFP installed in the SCORPIO focal reducer are presented. ... Velocity field . Mkn 1157 was observed 1 Sep. 2002 in the Ha emission line. Texp =32x240 sec, seeing 1.5", IFP260. ... This galaxy was observed September, 23 2000 in the Ha emission line, Texp=32x120 sec, seeing 2.5", IFP260. ... PV Cep was observed at the 6m telescope in May, 25 2003 in the [SII] 6716A with IFP501, Texp=36x200 sec, seeing 1.0". ...
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http://mavr.sao.ru/hq/lsfvo/devices/scorpio/galleries/gal_ifpnew.html -- 7.0 -- 28.12.2007
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http://www.sao.ru/hq/lsfvo/devices/scorpio/galleries/gal_ifpnew.html -- 7.0 -- 11.09.2010
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http://jet.sao.ru/hq/lsfvo/devices/scorpio/galleries/gal_ifpnew.html -- 7.0 -- 02.10.2012
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11. ASP: Big Clusters, Tiny Galaxies
home publications > mercury . ... Big Clusters, Tiny Galaxies . ... Astronomers struggle to understand why giant star clusters form in the tiniest of galaxies . ... These clusters are probably young versions of globular clusters, but they are commonly called super star clusters. Seven dwarf galaxies within 16 million light-years have formed super star clusters, with one of these galaxies, NGC 1569, possessing two young clusters. ... Super star clusters have a lot to tell us about star formation. ...
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http://www.astrosociety.org/pubs/mercury/32_03/clusters.html -- 17.5 -- 20.04.2012
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12. The 1 st Asian-Pacific Astronomy Olympiad
... The 1 st Asian-Pacific Astronomy Olympiad will held in Siberia (Asian part of Russian Federation) on December 4-11, 2005, a month later than the 10 th IAO in Beijing ). ... Only students did not participated at the IAO-2005 may participate in the APAO-2005 (that is a student may participate in the 10 th IAO in Beijing or in the 1 st APAO in Siberia but not in both of these Olympiads). For the 1 st APAO the (age) group of participants to be the same as proposed for IAO since 2006. i.e.: . ...
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http://www.issp.ac.ru/iao/apao/2005/2a.html -- 8.9 -- 16.09.2006
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13. ATNF Colloquium
ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Astrophysics graduate student programs . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Mopra radio telescope . ... The Australia Telescope National Facility Colloquium . ... The mass spectrum scales as N(M) ~ M^-1.5, similar to the mass spectra of young massive star clusters suggesting that individual molecular clouds are transformed in the starburst into individual star clusters. ...
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http://www.atnf.csiro.au/news/news.php?action=show_item&item_id=579 -- 28.1 -- 01.03.2014
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14. http://www.astro.louisville.edu/shared_skies/archive/select/ic/ic348/20121109/ic348_wikipedia_20130415.pdf
IC 348 1 IC 348 IC 348 Hubble image of IC 348 and its surroundings.[ ... References External links Amateur photography ( http ://www.photonhunter.at/IC348.html) Article Sources and Contributors 2 Article Sources and Contributors IC 348 Source: http ://en.wikipedia.org/w/index.php?oldid=549545123 Contributors : Jmencisom, PatrickHochleitner, RJHall Image Sources , Licenses and Contributors File:Hubble image of LRLL 54361 and its surroundings.tif Source: ...
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http://www.astro.louisville.edu/shared_skies/archive/select/ic/ic348/20121109/ic348_wikipedia_20130415.pdf -- 177.0 -- 15.04.2013
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15. Astrophysics Group AMI Publications
... Astrophysics Group . ... AMI Publications . ... AMI Consortium: Hurley-Walker N. et al., 2011, preprint (arXiv:1103.0947) . ... AMI Consortium: Olamaie M. et al., 2010, preprint (arXiv:1012.4996) . ... AMI Consortium: Shimwell T. W. et al., 2010, preprint (arXiv:1012.4441) . ... AMI Consortium: Davies et al., 2010, preprint (arXiv:1012.3659) . ... AMI Consortium: Franzen et al., 2010, preprint (arXiv:1012.3711) . ... AMI Consortium: Rodriguez-Gonzalvez C. et al., 2010, preprint (arXiv:1011.0325) . ...
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http://www.mrao.cam.ac.uk/facilities/ami/ami-publications/ -- 30.8 -- 10.04.2016
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16. A 1400-MHz Survey of 1478 Abell Clusters of Galaxies
... 87.1083Owen+ VIII/29 1400-MHz Survey of 1478 Abell Clusters of Galaxies (Owen+ 1982) ================================================================================ A 1400-MHz Survey of 1478 Abell Clusters of Galaxies Owen F.N., White R.A., Hilldrup K.C., Hanisch R.J. =1982AJ.. ... 0,] Major axis error 70- 71 A2 --- n_MajAxi *[ A, B, C,NR, ] Major axis note 73- 74 I2 arcmin MinAxi *? ... Note on dist-C: Ratio of the distance of the source from the cluster center to the corrected Abell cluster...
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http://www.sao.ru/cats/doc/CL_Owen82.html -- 9.3 -- 18.03.2015
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17. Region Algebra
... inclusive or left to right For example, to create a mask consisting of a large circle with a smaller box removed, one can use the and and not operators: CIRCLE(11,11,15) !BOX(11,11,3,6) and the resulting mask is: 1234567890123456789012345678901234567890 ---------------------------------------- 1:1111111111111111111111.. 2:1111111111111111111111.. 3:11111111111111111111111.. 4:111111111111111111111111.. ... 6:1111111111111111111111111.. ... 1111111111111.. ... 22:111111111111111111111.. ...
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http://hea-www.harvard.edu/RD/funtools/regalgebra.html -- 11.9 -- 01.10.2012
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18. Population of Galactic globular clusters, figures
... Galactocentric distance dependences of the physical parameters of globular clusters. ... The straight line in (a) is the rms regression. The large circles in (b) show mean masses within narrow R intervals, and the solid lines show the rms regression fits for thick-disk and old-halo (left) and young-halo and corona (right) clusters. The dashed lines in (c) and (d) are upper and lower envelopes drawn by eye. discussion in the text | privious figure | next figure . ...
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http://ip.rsu.ru/~marsakov/paper5/p5fg11_1.htm -- 2.2 -- 02.02.2007
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19. Astronomy HyperText Book: Stellar Clusters
Stellar Clusters are very useful laboratories for empirically studying stellar evolution. ... All cluster stars are at the same distance . All cluster stars have the same physical age . ... CM diagram Young Cluster In this case we see the Main Sequence fully represented. The blue dots represent massive stars with short main sequence lifetimes. ... Thus, identifying the most massive star which is still on the main sequence is an effective means of determining the age of a stellar cluster. ...
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http://zebu.uoregon.edu/textbook/sc.html -- 3.5 -- 23.01.1998
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20. Near-IR Imaging of Star-forming Regions with IRAF
... We report on our ongoing project ``Infrared Study of HII Regions Associated with Small Clouds.' ... These IR data, combined with optical imaging (which will be obtained from the IAC-80 telescope), IRAS survey maps, and existing CO observations of the associated clouds, will allow us to undertake a detailed investigation of the gas-to-dust mass ratio, initial mass function and the star-formation efficiency in these complexes. ... CHECKPSF: check the PSF (Point Spread Function) model, . ...
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http://www.adass.org/adass/proceedings/adass96/chans2.html -- 7.4 -- 23.06.1998
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