Poss-I 959 Poss-I 960 Poss-I 961 Poss-I 962 Poss-I 1009

Total Page:16

File Type:pdf, Size:1020Kb

Poss-I 959 Poss-I 960 Poss-I 961 Poss-I 962 Poss-I 1009 By Toshimi Taki, April 12, ’07 12h00m 98 11h30m 11h00m 122 ο P BB POSS-I 961 OSS-I 960 POSS-I 959 -35° Hydra -35° V919 3706 3573 2 3358 POSS-I 96 3568 3783 3557 ι 3742 3564 3749 Antlia POSS-I 1011 POSS-I 1010 S-I 1012 -40° POS 4112 -40° V361 X Centaurus 3680 POS S-I 1009 4219 V903 -45° -45° V785 V763 Vela 121 123 μ -50° δ -50° MW V359 PK 290+7.1 HP ρ HI HQ π V898 HH V369 3330 V348 U 3960 V885 -55° 4230 -55° V419 SV BH 3918 PK 285+1.1 γ Crux V537 Tr 19 VY I.2581 C91 (3532) Stock 13 3293 PK 288 4337 δ ο Tr 17 +0.1 3324 3247 W PK 293+ 1.1 U BG BL Hogg 14 YZ AG HR CH LZ Cr 223 AG 4439 ε DG 3603 C92 (3372) -60° Cr 236 -60° VZ Harvard 5 4103 C97 Ru 93 Tr 20 R RS IT Ru 92 (3766) Bochum 12 V510 ι 4349 BY BO λ V530 T Ru 97 I.2714 Carina Stock 14 V529 140 C100 (Cr 249) Note: Detail of Carinae and vicinity is shown in Chart No.A3. Magnitude 0 1 2 3 4 5 6 7 8 8.5 Scale By Toshimi Taki, Aug. 6, ’06 11h00m 99 10h30m 10h00m 123 BB 3281 AU 3224 OSS-I 959 POSS-I 9352869 P 3289 3267 POSS-I 957 -35° 3271 3268 -35° 3273 3258 3347 η 3358 3275 3573 60 POSS-I 9 AV 3568 ι 3564 3557 Antlia U 3278 3244 POSS-I POSS-I 1009 3250 1008 1010 POSS-I 3250E -40° C74 (3132) -40° V361 3318 3256 3366 3263 PO SS-I 100 3261 V339 7 -45° V903 V341 -45° C79 (3201) 122 Vela QX 124 V345 μ V337 -50° Cr 213 QY -50° GY 2999 MW 3228 V359 HP Centaurus Y PK 290+7.1 HI V348 MS Pismis 16 HQ HH 2910 V346 W Z Ru 82 2925 3330 φ V898 3105 Ru 79 GL GZ Ru 83 π RY -55° QW -55° SV PK 285+1.1 I.2581 PK 279-3.1 3033 VY 2899 V419 PK 283-1.1 V366 I.2488 Tr 19 3247 3293 QY V490 V537 C91 (3532) PK 288+0.1 Y PK 278-4.1 3324 QX Stock 13 Tr 17 V368 ER YZ U V480 C90 (2867) BO Cr 223 HR ο AG Bochum 9 3114 PK 293+1.1 C92 (3372) Tr 12 ι I.2501 Cr 236 -60° V510 -60° Tr 11 Ru 93 Ru 92 S Bochum 12 3603IT RS Carina I V530 3211 C97 (3766) I.2714 V529 140 Note: Detail of Carinae and vicinity is shown in Chart No.A3. Magnitude 0 1 2 3 4 5 6 7 8 8.5 Scale By Toshimi Taki, May 9, ’07 10h00m 100 9h30m 9h00m 124 POSS-I 956 POSS-I 957 POSS-I 9 55 -35° -35° Pyxis η ε 2818A 2818 Antlia 2845 POSS-I 1007 POSS-I 1006 08 OSS-I 10 ψ -40° P -40° GP C74 (3132) Tr 10 Cr 197 PT λ Ru 67 V339 S Vela 2659 -45° U Pismis 12 -45° V341 Bochum 7 C79 (3201) Waterloo 6 SX Pismis 8 Pismis 6 2660 MN QX SW T 123 125 Mrk 18 I.2395 V345 2670 FY QY 2999 2866 -50° V337 Cr 213 -50° BG QT GY CV Y 3228 MS Pismis 16 2910 Harvard 3 Ru 79 2925 IK C85 (I.2391) Ru 82 2669 V348 Z φ W 3105 Ru 83 δ V346 κ QW NT GZ RY V -55° 2899 -55° 3033 I.2488 I.2581 PK 279 -3.1 PK 278-4.1 V490 C90 (2867) QY QX V475 V477 3247 V480 3293 V368 Y ι 3324 PK 283-1.1 YZ HR X 3114 I.2501 Cr 223 Tr 12 ε V -60° Bochum 9 Carina -60° V515 Tr 11 V466 V510 S I R 3211 141 Magnitude 0 1 2 3 4 5 6 7 8 8.5 Scale By Toshimi Taki, Aug. 13, ’06 9h00m 101 8h30m 8h00m 125 RS V416 SS-I 954 P POSS-I 955 PO OSS-I 953 -35° Pyxis β 2579 V427 -35° Cr 185 MX 2818A AB AT 2818 PQ C71 (2477) 2451 2546 Puppis AS Pismis 5 NO PO POSS-I 1005 SS-I 1004 ζ 006 POSS-I 1 GO -40° AP -40° GP AU Cr 197 ESO 311-G012 Tr 10 BH W PT λ Ru 67 RZ Pismis 4 AI 2659 Waterloo 6 -45° Bochum 7 -45° Pismis 12 Vela SX Pismis 6 AH Pismis 8 2660 MN γ SW T AX I.2395 124 2427 126 PK 264-8.1 Cr 173 Mrk 18 2670 MY 2547 FY V V406 -50° -50° 2866 BG CV PK 264-12.1 QT Harvard 3 C85 (I.2391) Y 2669 χ 2910 IK δ GL NT -55° κ -55° V 2899 V467 I.2488 Carina V377 V475 PK 278-4.1 C90 (2867) V477 ε V341 X V480 ι V V466 V3C5966 (2516) -60° I.2501 -60° V393 V455 2417 141 Magnitude 0 1 2 3 4 5 6 7 8 8.5 Scale By Toshimi Taki, Aug. 13, ’06 8h00m 102 7h30m 7h00m 126 V416 3 V361 PROSSS-I 95 POSS-I 952 POSS-I 951 -35° -35° V427 MX 2296 CH V374 NV Cr 135 AT 2451 π PQ 2546 C71 (2477) P POSS-I 1003 OSS-I 1002 04 POSS-I 10 -40° ζ AP -40° ESO 311-G012 2310 NP AU BH W Puppis σ L2 AI -45° Cr 173 -45° AH Mel 66 γ 2427 AX MY 125 V366 127 PK 264-8.1 V 2547 V406 τ -50° -50° Vela PK 264-12.1 χ NT -55° V448 -55° V467 ν Carina μ V341 V452 ε Pictor X V466 C96 (2516) V -60° -60° V393 V455 2417 2369 α 142 Magnitude 0 1 2 3 4 5 6 7 8 8.5 Scale By Toshimi Taki, Aug. 13, ’06 7h00m 103 6h30m 6h00m 2090 127 951 POVS36S1-I POSS-I 950 POSSκ-I 949 -35° -35° γ 2296 CH β POSS-I 948 θ ξ Cr 135 Columba POSS-I 1001 POSS-I 1000 02 POSS-I 10 -40° AF -40° 2310 π1 NP π2 η ν L2 -45° -45° Puppis XX 126 128 V366 τ -50° -50° V444 β 2191 α Carina δ V448 -55° -55° ν γ κ μ Pictor ZZ V452 λ -60° -60° α V455 2369 Dorado 2417 β 142 Magnitude 0 1 2 3 4 5 6 7 8 8.5 Scale By Toshimi Taki, Aug. 13, ’06 6h00m 104 5h30m 5h00m 128 S-I 949 POSS-I 948 POSS-I 947ο POSS-I POS 946 -35° -35° γ ε γ1 γ2 β 1827 Caelum ξ θ 1808 1792 Columba POSS-I 999 POSS-I 998 1000 POSS-I SW C73 (1851) -40° -40° AF π2 α η π1 WW -45° -45° Puppis 1930 T XX Pictor 127 129 S η1 η2 UZ R ζ -50° λ -50° β V444 θ 2191 α 1705 ι Carina 1617 δ 1596 SU -55° κ α -55° γ VY ν ζ 1574 Dorado λ μ ZZ 1703 1688 1672 κ ε AL -60° 1796 -60° I.2056 R β α Reticulum 143 Magnitude 0 1 2 3 4 5 6 7 8 8.5 Scale By Toshimi Taki, Aug. 14, ’06 5h00m 105 4h30m 4h00m 129 POSS-I 946 POSS-I 945 POSS-I 944 -35° γ1 -35° γ2 I.2006 47 POSS-I 9 1827 β 1460 1808 Columba 1792 R POSS-I 997 POSS-I 9E9r6idanus 98 POSS-I 9 GL Caelum -40° GM -40° C73 (1851) 1572 α δ α EU 1487 1570 1512 FZ GI WW δ 1558 1411 I.2035 1448 -45° U -45° 1493 Pictor Horologium T 1433 1527 128 1567 130 η1 S I.2000 R 1494 η2 UZ λ -50° -50° ζ γ I.1954 WX θ 1705 ι 1617 1515 1596 UX α 1566 SU 1549 1553 -55° 1533 -55° 1546 VY 1536 κ 1574 ζ 1543 Dorado 1672 Reticulum 1703 1688 κ ε λ I.2056 AL ι -60° 1796 -60° R δ α γ 1559 R η θ β 143 Magnitude 0 1 2 3 4 5 6 7 8 8.5 Scale By Toshimi Taki, Aug. 14, ’06 4h00m 106 1380A 3h30m 3h00m 130 1351 1380 1374 SS-I 944 1399 PO13S7S5 -I 943 PO PO 1427 χ2 SS-I 942 -35° 1381 1336 TZ -35° 1379 I.2006 η3 1437 1387 χ1 χ3 1326 η1 1404 1365 Fornax η2 1386 I 945 1389 1317 POSS- 1460 1310 1341 1316 SS-I 995 POSS-I 9 PO 94 1217 6 ψ POSS-I 99 GL GM -40° -40° 1291 θ EU δ 1487 α FZ Eridanus GI 1512 1411 1448 Ca-e4lu5m° I.2035 1558 U -45° 1493 1433 1527 129 I.2000 131 1567 1494 R Dorado -50° T -50° I.1954 ι Horologium γ WX I.1933 XY 1249 η 1515 UX ζ 1617 C87 (1261) 1596 1566 1549 -55° 1533 -55° α 1553 1546 1536 1574 TW 1543 Reticulum μ ε I.2056 ι -60° -60° λ δ ζ2 γ ζ1 R ν α κ 1559 WZ 144 Magnitude 0 1 2 3 4 5 6 7 8 8.5 Scale By Toshimi Taki, Aug. 14, ’06 3h00m 107 2h30m 2h00m 131 POSS-I 942 POSS-I 941 POSS-I 940 -35° η3 -35° η TZ 1 AD η2 Fornax Sculptor POSS-I 992 ψ POSS-I 993 94 POSS-I 19217 986 ι -40° θ -40° 1291 φ χ -45° Phoenix -45° ψ Eridanus κ 130 132 R AE -50° T ι -50° φ χ η XY 685 I.1933 1249 Horologium ζ C87 (1261) -55° -55° TW 782 α Reticulum μ 484 λ -60° -60° α ζ2 ν Hydrus Tucana ζ1 WZ 144 Magnitude 0 1 2 3 4 5 6 7 8 8.5 Scale By Toshimi Taki, Aug.
Recommended publications
  • 500 Natural Sciences and Mathematics
    500 500 Natural sciences and mathematics Natural sciences: sciences that deal with matter and energy, or with objects and processes observable in nature Class here interdisciplinary works on natural and applied sciences Class natural history in 508. Class scientific principles of a subject with the subject, plus notation 01 from Table 1, e.g., scientific principles of photography 770.1 For government policy on science, see 338.9; for applied sciences, see 600 See Manual at 231.7 vs. 213, 500, 576.8; also at 338.9 vs. 352.7, 500; also at 500 vs. 001 SUMMARY 500.2–.8 [Physical sciences, space sciences, groups of people] 501–509 Standard subdivisions and natural history 510 Mathematics 520 Astronomy and allied sciences 530 Physics 540 Chemistry and allied sciences 550 Earth sciences 560 Paleontology 570 Biology 580 Plants 590 Animals .2 Physical sciences For astronomy and allied sciences, see 520; for physics, see 530; for chemistry and allied sciences, see 540; for earth sciences, see 550 .5 Space sciences For astronomy, see 520; for earth sciences in other worlds, see 550. For space sciences aspects of a specific subject, see the subject, plus notation 091 from Table 1, e.g., chemical reactions in space 541.390919 See Manual at 520 vs. 500.5, 523.1, 530.1, 919.9 .8 Groups of people Add to base number 500.8 the numbers following —08 in notation 081–089 from Table 1, e.g., women in science 500.82 501 Philosophy and theory Class scientific method as a general research technique in 001.4; class scientific method applied in the natural sciences in 507.2 502 Miscellany 577 502 Dewey Decimal Classification 502 .8 Auxiliary techniques and procedures; apparatus, equipment, materials Including microscopy; microscopes; interdisciplinary works on microscopy Class stereology with compound microscopes, stereology with electron microscopes in 502; class interdisciplinary works on photomicrography in 778.3 For manufacture of microscopes, see 681.
    [Show full text]
  • A Gaia DR 2 and VLT/FLAMES Search for New Satellites of The
    Astronomy & Astrophysics manuscript no. spec_v1_ref1_arx c ESO 2019 February 14, 2019 A Gaia DR 2 and VLT/FLAMES search for new satellites of the LMC⋆ T. K. Fritz1, 2, R. Carrera3, G. Battaglia1, 2, and S. Taibi1, 2 1 Instituto de Astrofisica de Canarias, calle Via Lactea s/n, E-38205 La Laguna, Tenerife, Spain e-mail: [email protected] 2 Universidad de La Laguna, Dpto. Astrofisica, E-38206 La Laguna, Tenerife, Spain 3 INAF - Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, I-35122 Padova, Italy ABSTRACT A wealth of tiny galactic systems populates the surroundings of the Milky Way. However, some of these objects might actually have their origin as former satellites of the Magellanic Clouds, in particular of the LMC. Examples of the importance of understanding how many systems are genuine satellites of the Milky Way or the LMC are the implications that the number and luminosity/mass function of satellites around hosts of different mass have for dark matter theories and the treatment of baryonic physics in simulations of structure formation. Here we aim at deriving the bulk motions and estimates of the internal velocity dispersion and metallicity properties in four recently discovered distant southern dwarf galaxy candidates, Columba I, Reticulum III, Phoenix II and Horologium II. We combine Gaia DR2 astrometric measurements, photometry and new FLAMES/GIRAFFE intermediate resolution spectroscopic data in the region of the near-IR Ca II triplet lines; such combination is essential for finding potential member stars in these low luminosity systems. We find very likely member stars in all four satellites and are able to determine (or place limits on) the systems bulk motions and average internal properties.
    [Show full text]
  • Naming the Extrasolar Planets
    Naming the extrasolar planets W. Lyra Max Planck Institute for Astronomy, K¨onigstuhl 17, 69177, Heidelberg, Germany [email protected] Abstract and OGLE-TR-182 b, which does not help educators convey the message that these planets are quite similar to Jupiter. Extrasolar planets are not named and are referred to only In stark contrast, the sentence“planet Apollo is a gas giant by their assigned scientific designation. The reason given like Jupiter” is heavily - yet invisibly - coated with Coper- by the IAU to not name the planets is that it is consid- nicanism. ered impractical as planets are expected to be common. I One reason given by the IAU for not considering naming advance some reasons as to why this logic is flawed, and sug- the extrasolar planets is that it is a task deemed impractical. gest names for the 403 extrasolar planet candidates known One source is quoted as having said “if planets are found to as of Oct 2009. The names follow a scheme of association occur very frequently in the Universe, a system of individual with the constellation that the host star pertains to, and names for planets might well rapidly be found equally im- therefore are mostly drawn from Roman-Greek mythology. practicable as it is for stars, as planet discoveries progress.” Other mythologies may also be used given that a suitable 1. This leads to a second argument. It is indeed impractical association is established. to name all stars. But some stars are named nonetheless. In fact, all other classes of astronomical bodies are named.
    [Show full text]
  • The Constellation Microscopium, the Microscope Microscopium Is A
    The Constellation Microscopium, the Microscope Microscopium is a small constellation in the southern sky, defined in the 18th century by Nicolas Louis de Lacaille in 1751–52 . Its name is Latin for microscope; it was invented by Lacaille to commemorate the compound microscope, i.e. one that uses more than one lens. The first microscope was invented by the two brothers, Hans and Zacharius Jensen, Dutch spectacle makers of Holland in 1590, who were also involved in the invention of the telescope (see below). Lacaille first showed it on his map of 1756 under the name le Microscope but Latinized this to Microscopium on the second edition published in 1763. He described it as consisting of "a tube above a square box". It contains sixty-nine stars, varying in magnitude from 4.8 to 7, the lucida being Gamma Microscopii of apparent magnitude 4.68. Two star systems have been found to have planets, while another has a debris disk. The stars that now comprise Microscopium may formerly have belonged to the hind feet of Sagittarius. However, this is uncertain as, while its stars seem to be referred to by Al-Sufi as having been seen by Ptolemy, Al-Sufi does not specify their exact positions. Microscopium is bordered Capricornus to the north, Piscis Austrinus and Grus to the west, Sagittarius to the east, Indus to the south, and touching on Telescopium to the southeast. The recommended three-letter abbreviation for the constellation, as adopted Seen in the 1824 star chart set Urania's Mirror (lower left) by the International Astronomical Union in 1922, is 'Mic'.
    [Show full text]
  • Educator's Guide: Orion
    Legends of the Night Sky Orion Educator’s Guide Grades K - 8 Written By: Dr. Phil Wymer, Ph.D. & Art Klinger Legends of the Night Sky: Orion Educator’s Guide Table of Contents Introduction………………………………………………………………....3 Constellations; General Overview……………………………………..4 Orion…………………………………………………………………………..22 Scorpius……………………………………………………………………….36 Canis Major…………………………………………………………………..45 Canis Minor…………………………………………………………………..52 Lesson Plans………………………………………………………………….56 Coloring Book…………………………………………………………………….….57 Hand Angles……………………………………………………………………….…64 Constellation Research..…………………………………………………….……71 When and Where to View Orion…………………………………….……..…77 Angles For Locating Orion..…………………………………………...……….78 Overhead Projector Punch Out of Orion……………………………………82 Where on Earth is: Thrace, Lemnos, and Crete?.............................83 Appendix………………………………………………………………………86 Copyright©2003, Audio Visual Imagineering, Inc. 2 Legends of the Night Sky: Orion Educator’s Guide Introduction It is our belief that “Legends of the Night sky: Orion” is the best multi-grade (K – 8), multi-disciplinary education package on the market today. It consists of a humorous 24-minute show and educator’s package. The Orion Educator’s Guide is designed for Planetarians, Teachers, and parents. The information is researched, organized, and laid out so that the educator need not spend hours coming up with lesson plans or labs. This has already been accomplished by certified educators. The guide is written to alleviate the fear of space and the night sky (that many elementary and middle school teachers have) when it comes to that section of the science lesson plan. It is an excellent tool that allows the parents to be a part of the learning experience. The guide is devised in such a way that there are plenty of visuals to assist the educator and student in finding the Winter constellations.
    [Show full text]
  • Snake in the Clouds: a New Nearby Dwarf Galaxy in the Magellanic Bridge ∗ Sergey E
    MNRAS 000, 1{21 (2018) Preprint 19 April 2018 Compiled using MNRAS LATEX style file v3.0 Snake in the Clouds: A new nearby dwarf galaxy in the Magellanic bridge ∗ Sergey E. Koposov,1;2 Matthew G. Walker,1 Vasily Belokurov,2;3 Andrew R. Casey,4;5 Alex Geringer-Sameth,y6 Dougal Mackey,7 Gary Da Costa,7 Denis Erkal8, Prashin Jethwa9, Mario Mateo,10, Edward W. Olszewski11 and John I. Bailey III12 1McWilliams Center for Cosmology, Carnegie Mellon University, 5000 Forbes Ave, 15213, USA 2Institute of Astronomy, University of Cambridge, Madingley road, CB3 0HA, UK 3Center for Computational Astrophysics, Flatiron Institute, 162 5th Avenue, New York, NY 10010, USA 4School of Physics and Astronomy, Monash University, Clayton 3800, Victoria, Australia 5Faculty of Information Technology, Monash University, Clayton 3800, Victoria, Australia 6Astrophysics Group, Physics Department, Imperial College London, Prince Consort Rd, London SW7 2AZ, UK 7Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia 8Department of Physics, University of Surrey, Guildford, GU2 7XH, UK 9European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching, Germany 10Department of Astronomy, University of Michigan, 311 West Hall, 1085 S University Avenue, Ann Arbor, MI 48109, USA 11Steward Observatory, The University of Arizona, 933 N. Cherry Avenue., Tucson, AZ 85721, USA 12Leiden Observatory, Leiden University, Niels Bohrweg 2, 2333 CA Leiden, The Netherlands Accepted XXX. Received YYY; in original form ZZZ ABSTRACT We report the discovery of a nearby dwarf galaxy in the constellation of Hydrus, between the Large and the Small Magellanic Clouds. Hydrus 1 is a mildy elliptical ultra-faint system with luminosity MV 4:7 and size 50 pc, located 28 kpc from the Sun and 24 kpc from the LMC.
    [Show full text]
  • These Sky Maps Were Made Using the Freeware UNIX Program "Starchart", from Alan Paeth and Craig Counterman, with Some Postprocessing by Stuart Levy
    These sky maps were made using the freeware UNIX program "starchart", from Alan Paeth and Craig Counterman, with some postprocessing by Stuart Levy. You’re free to use them however you wish. There are five equatorial maps: three covering the equatorial strip from declination −60 to +60 degrees, corresponding roughly to the evening sky in northern winter (eq1), spring (eq2), and summer/autumn (eq3), plus maps covering the north and south polar areas to declination about +/− 25 degrees. Grid lines are drawn at every 15 degrees of declination, and every hour (= 15 degrees at the equator) of right ascension. The equatorial−strip maps use a simple rectangular projection; this shows constellations near the equator with their true shape, but those at declination +/− 30 degrees are stretched horizontally by about 15%, and those at the extreme 60−degree edge are plotted twice as wide as you’ll see them on the sky. The sinusoidal curve spanning the equatorial strip is, of course, the Ecliptic −− the path of the Sun (and approximately that of the planets) through the sky. The polar maps are plotted with stereographic projection. This preserves shapes of small constellations, but enlarges them as they get farther from the pole; at declination 45 degrees they’re about 17% oversized, and at the extreme 25−degree edge about 40% too large. These charts plot stars down to magnitude 5, along with a few of the brighter deep−sky objects −− mostly star clusters and nebulae. Many stars are labelled with their Bayer Greek−letter names. Also here are similarly−plotted maps, based on galactic coordinates.
    [Show full text]
  • May 30 2012 Stars2 FASI Book
    Summary You now know the four Guidepost You are also on your way to learning more constellations: Orion, The Big Dipper, The advanced astronomy. Swan, and Cassiopeia. In Book 3 of this series, Seasons & the Round and round they go, year after Celestial Sphere, we expand our presentation year. The jealous Big Dipper follows Orion, to three dimensions. This will enable you to the thirsty Swan fies after the Big Dipper, understand the seasons, the way sundials tell Cassiopeia the queen pursues the beautiful time, and the entire celestial sphere of stars. Swan, and Orion chases the queen. Here we introduce the Horizon Globe, which is a device that simulates what you see on the You also know when Orion is by the Sun, celestial sphere. It’s like going to a 3-D movie, which allows you to know where and when to except you won’t have to wear the glasses! look for your favorite constellations. After these three introductory books, you You’ve heard the Four (expanded) Stories, will be ready to quantify what you observe in which helps you fnd other interesting stars near the sky. We’ll measure angles and estimate the Guidepost constellations. distances to the Sun and Moon. We’ll estimate the size of the Earth, Moon and Sun. These You know about the North Star, and how to measurements will make it possible to develop fnd it from any of the Guideposts. You’ve seen theories that explain the observations. the Zodiac, which is interesting because the most important object in the sky—the Sun— As a reminder of what was covered in this goes through these star constellations.
    [Show full text]
  • 81 Southern Objects for a 10” Telescope. 0-4Hr 4-8Hr 8-12Hr
    81 southern objects for a 10” telescope. 0-4hr NGC55|00h 15m 22s|-39 11’ 35”|33’x 5.6’|Sculptor|Galaxy| NGC104|00h 24m 17s|-72 03’ 30”|31’|Tucana|Globular NGC134|00h 30m 35s|-33 13’ 00”|8.5’x2’|Sculptor|Galaxy| ESO350-40|00h 37m 55s|-33 41’ 20”|1.5’x1.2’|Sculptor|Galaxy|The Cartwheel NGC300|00h 55m 06s|-37 39’ 24”|22’x15.5’|Sculptor|Galaxy| NGC330|00h 56m 27s|-72 26’ 37”|Tucana|1.9’|SMC open cluster| NGC346|00h 59m 14s|-72 09’ 19”|Tucana|5.2’|SMC Neb| ESO351-30|01h 00m 22s|-33 40’ 50”|60’x56’|Sculptor|Galaxy|Sculptor Dwarf NGC362|01h 03m 23s|-70 49’ 42”|13’|Tucana|Globular| NGC2573| 01h 37m 21s|-89 25’ 49”|Octans| 2.0x 0.8|galaxy|polarissima australis| NGC1049|02h 39m 58s|-34 13’ 52”|24”|Fornax|Globular| ESO356-04|02h 40m 09s|-34 25’ 43”|60’x100’|Fornax|Galaxy|Fornax Dwarf NGC1313|03h 18m 18s|-66 29’ 02”|9.1’x6.3’|Reticulum|Galaxy| NGC1316|03h 22m 51s|-37 11’ 22”|12’x8.5’|Fornax|Galaxy| NGC1365|03h 33m 46s|-36 07’ 13”|11.2’x6.2’|Fornax|Galaxy NGC1433|03h 42m 08s|-47 12’ 18”|6.5’x5.9’|Horologium|Galaxy| 4-8hr NGC1566|04h 20m 05s|-54 55’ 42”|Dorado|Galaxy| Reticulum Dwarf|04h 31m 05s|-58 58’ 00”|Reticulum|LMC globular| NGC1808|05h 07m 52s|-37 30’ 20”|6.4’x3.9’|Columba|Galaxy| Kapteyns Star|05h 11m 35s|-45 00’ 16”|Stellar|Pictor|Nearby star| NGC1851|05h 14m 15s|-40 02’ 30”|11’|Columba|Globular| NGC1962group|05h 26m 17s|-68 50’ 28”|?| Dorado|LMC neb/cluster NGC1968group|05h 27m 22s|-67 27’ 36”|12’ for group|Dorado| LMC Neb/cluster| NGC2070|05h 38m 37s|-69 05’ 52”|11’|Dorado|LMC Neb|Tarantula| NGC2442|07h 36m 24s|-69 32’ 38”|5.5’x4.9’|Volans|Galaxy|The meat hook| NGC2439|07h 40m 59s|-31 38’36”|10’|Puppis|Open Cluster| NGC2451|07h 45m 35s|-37 57’ 27”|45’|Puppis|Open Cluster| IC2220|07h 56m 57s|-59 06’ 00”|6’x4’|Carina|Nebula|Toby Jug| NGC2516|07h 58m 29s|-60 51’ 46”|29’|Carina|Open Cluster 8-12hr NGC2547|08h 10m 50s|-49 15’ 39”|20’|Vela|Open Cluster| NGC2736|09h 00m 27s|-45 57’ 49”|30’x7’|Vela|SNR|The Pencil| NGC2808|09h 12m 08s|-64 52’ 48”|12’|Carina|Globular| NGC2818|09h 16m 11s|-36 35’ 59”|9’|Pyxis|Open Cluster with planetary.
    [Show full text]
  • Morphology and Large-Scale Structure Within the Horologium-Reticulum Supercluster of Galaxies
    Morphology and Large-Scale Structure within the Horologium-Reticulum Supercluster of Galaxies Matthew Clay Fleenor A dissertation submitted to the faculty of the University of North Carolina at Chapel Hill in partial fulfillment of the requirements for the degree of Doctor of Philosophy in the Department of Physics & Astronomy. Chapel Hill 2006 Approved by Advisor: James A. Rose Reader: Gerald Cecil Reader: Wayne A. Christiansen Reader: Dan Reichart Reader: Paul Tiesinga c 2006 Matthew Clay Fleenor ii ABSTRACT Matthew Clay Fleenor: Morphology and Large-Scale Structure within the Horologium-Reticulum Supercluster of Galaxies (Under the Direction of James A. Rose) We have undertaken a comprehensive spectroscopic survey of the Horologium-Reticulum supercluster (HRS) of galaxies. With a concentration on the intercluster regions, our goal is to resolve the “cosmic web” of filaments, voids, and sheets within the HRS and to examine the interrelationship between them. What are the constituents of the HRS? What can be understood about the formation of such a behemoth from these current constituents? More locally, are there small-scale imprints of the larger, surrounding environment, and can we relate the two with any confidence? What is the relationship between the HRS and the other superclusters in the nearby universe? These are the questions driving our inquiry. To answer them, we have obtained over 2500 galaxy redshifts in the direction of the intercluster regions in the HRS. Specifically, we have developed a sample of galaxies with a limiting brightness of bJ < 17.5, which samples the galaxy luminosity function down to one magnitude below M⋆ at the mean redshift of the HRS,z ¯ ≈ 0.06.
    [Show full text]
  • THE SKY TONIGHT Constellation Is Said to Represent Ganymede, the Handsome Prince of Capricornus Troy
    - October Oketopa HIGHLIGHTS Aquarius and Aquila In Greek mythology, the Aquarius THE SKY TONIGHT constellation is said to represent Ganymede, the handsome prince of Capricornus Troy. His good looks attracted the attention of Zeus, who sent the eagle The Greeks associated Capricornus Aquila to kidnap him and carry him with Aegipan, who was one of the to Olympus to serve as a cupbearer Panes - a group of half-goat men to the gods. Because of this story, who often had goat legs and horns. Ganymede was sometimes seen as the god of homosexual relations. He Aegipan assumed the form of a fish- also gives his name to one of the tailed goat and fled into the ocean moons of Jupiter, which are named to flee the great monster Typhon. after the lovers of Zeus. Later, he aided Zeus in defeating Typhon and was rewarded by being To locate Aquarius, first find Altair, placed in the stars. the brightest star in the Aquila constellation. Altair is one of the To find Capricornus (highlighted in closest stars to Earth that can be seen orange on the star chart), first locate with the naked eye, at a distance the Aquarius constellation, then of 17 light years. From Altair, scan look to the south-west along the east-south-east to find Aquarius ecliptic line (the dotted line on the (highlighted in yellow on the star chart). star chart). What’s On in October? October shows at Perpetual Guardian Planetarium, book at Museum Shop or online. See website for show times and - details: otagomuseum.nz October Oketopa SKY GUIDE Capturing the Cosmos Planetarium show.
    [Show full text]
  • Useful Constellation Lists and More
    USEFUL CONSTELLATION LISTS AND MORE The 12 Star Signs (Zodiac Signs) Aries, Gemini, Taurus, Cancer, Leo, Virgo, Libra, Scorpio, Sagittarius, Capricorn, Aquarius, Pieces. Constellations According to month, when they are seen at their best (9pm) meaning at their highest point January - Caelum, Dorado, Mensa, Orion, Reticulum, Taurus February - Auriga, Camelopardalis, Canis Major, Columba, Gemini, Lepus, Monoceros, Pictor March - Cancer, Canis Minor, Carina, Lynx, Puppis, Pyxis, Vela, Volans April - Antlia, Chamaeleon, Crater, Hydra, Leo, Leo Minor, Sextans, Ursa Major May - Canes Venatici, Centaurus, Coma Berenices, Corvus, Crux, Musca, Virgo June - Boötes, Circinus, Libra, Lupus, Ursa Minor July - Apus, Ara, Corona Borealis, Draco, Hercules, Norma, Ophiuchus, Scorpius, Serpens, Triangulum Australe August - Corona Austrina, Lyra, Sagittarius, Scutum, Telescopium September - Aquila, Capricornus, Cygnus, Delphinus, Equuleus, Indus, Microscopium, Pavo, Sagitta, Vulpecula October - Aquarius, Cepheus, Grus, Lacerta, Octans, Pegasus, Piscis Austrinus November - Andromeda, Cassiopeia, Phoenix, Pisces, Sculptor, Tucana December - Aries, Cetus, Eridanus, Fornax, Horologium, Hydrus, Perseus, Triangulum Months January – named in honour of the Roman god Janus the protector of doors February – named derived from the Roman verb ‘februum’ which means to cleanse. March – named in honour of Mars, the Roman God of war. April – named derived from the Latin word ‘aperiō’, to bud, to open (for buds) May – named after the Roman goddess Maia, Goddess of Spring
    [Show full text]