The Relation Between Globular Cluster Systems and Supermassive Black
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2014 Observers Challenge List
2014 TMSP Observer's Challenge Atlas page #s # Object Object Type Common Name RA, DEC Const Mag Mag.2 Size Sep. U2000 PSA 18h31m25s 1 IC 1287 Bright Nebula Scutum 20'.0 295 67 -10°47'45" 18h31m25s SAO 161569 Double Star 5.77 9.31 12.3” -10°47'45" Near center of IC 1287 18h33m28s NGC 6649 Open Cluster 8.9m Integrated 5' -10°24'10" Can be seen in 3/4d FOV with above. Brightest star is 13.2m. Approx 50 stars visible in Binos 18h28m 2 NGC 6633 Open Cluster Ophiuchus 4.6m integrated 27' 205 65 Visible in Binos and is about the size of a full Moon, brightest star is 7.6m +06°34' 17h46m18s 2x diameter of a full Moon. Try to view this cluster with your naked eye, binos, and a small scope. 3 IC 4665 Open Cluster Ophiuchus 4.2m Integrated 60' 203 65 +05º 43' Also check out “Tweedle-dee and Tweedle-dum to the east (IC 4756 and NGC 6633) A loose open cluster with a faint concentration of stars in a rich field, contains about 15-20 stars. 19h53m27s Brightest star is 9.8m, 5 stars 9-11m, remainder about 12-13m. This is a challenge obJect to 4 Harvard 20 Open Cluster Sagitta 7.7m integrated 6' 162 64 +18°19'12" improve your observation skills. Can you locate the miniature coathanger close by at 19h 37m 27s +19d? Constellation star Corona 5 Corona Borealis 55 Trace the 7 stars making up this constellation, observe and list the colors of each star asterism Borealis 15H 32' 55” Theta Corona Borealis Double Star 4.2m 6.6m .97” 55 Theta requires about 200x +31° 21' 32” The direction our Sun travels in our galaxy. -
Observing Galaxies in Pegasus 01 October 2015 23:07
Observing galaxies in Pegasus 01 October 2015 23:07 Context As you look towards Pegasus you are looking below the galactic plane under the Orion spiral arm of our galaxy. The Perseus-Pisces supercluster wall of galaxies runs through this constellation. It stretches from RA 3h +40 in Perseus to 23h +10 in Pegasus and is around 200 million light years away. It includes the Pegasus I group noted later this document. The constellation is well placed from mid summer to late autumn. Pegasus is a rich constellation for galaxy observing. I have observed 80 galaxies in this constellation. Relatively bright galaxies This section covers the galaxies that were visible with direct vision in my 16 inch or smaller scopes. This list will therefore grow over time as I have not yet viewed all the galaxies in good conditions at maximum altitude in my 16 inch scope! NGC 7331 MAG 9 This is the stand out galaxy of the constellation. It is similar to our milky way. Around it are a number of fainter NGC galaxies. I have seen the brightest one, NGC 7335 in my 10 inch scope with averted vision. I have seen NGC 7331 in my 25 x 100mm binoculars. NGC 7814 - Mag 10 ? Not on observed list ? This is a very lovely oval shaped galaxy. By constellation Page 1 NGC 7332 MAG 11 / NGC 7339 MAG 12 These galaxies are an isolated bound pair about 67 million light years away. NGC 7339 is the fainter of the two galaxies at the eyepiece. I have seen NGC 7332 in my 25 x 100mm binoculars. -
View the Energy Map of Trinidad and Tobago, 2017 Edition
Trinidad and Tobago LNG export destinations 2015 (million m3 of LNG) Trinidad and Tobago deepwater area for development 60°W 59°W 58°W Trinidad and Tobago territorial waters ENERGY MAP OF TRINIDAD AND TOBAGO 1000 2000 m m 2017 edition GRENADA BARBADOS Trinidad and Tobago 2000m LNG to Europe A tlantic Ocean 2.91 million m3 LNG A TLANTIC Caribbean 2000m 20 Produced by Petroleum Economist, in association with 00 O CEAN EUROPE Sea m Trinidad and Tobago 2000m LNG to North America NORTH AMERICA Trinidad and Tobago 5.69 million m3 LNG LNG to Asia 3 GO TTDAA 30 TTDAA 31 TTDAA 32 BA 1.02 million m LNG TO Trinidad and Tobago OPEN OPEN OPEN 12°N LNG to MENA 3 1.90 million m LNG ASIA Trinidad and Tobago CARIBBEAN TRINIDAD AND TOBAGO 2000m LNG to Caribbean Atlantic LNG Company profile Company Profile Company profile Company Profile 3 Established by the Government of Trinidad and Tobago in August 1975, The National Gas Company of Trinidad and Tobago Limited (NGC) is an BHP Billiton is a leading global resources company with a Petroleum Business that includes exploration, development, production and marketing Shell has been in Trinidad and Tobago for over 100 years and has played a major role in the development of its oil and gas industry. Petroleum Company of Trinidad and Tobago Limited (Petrotrin) is an integrated Oil and Gas Company engaged in the full range of petroleum 3.84 million m LNG internationally investment-graded company that is strategically positioned in the midstream of the natural gas value chain. -
Making a Sky Atlas
Appendix A Making a Sky Atlas Although a number of very advanced sky atlases are now available in print, none is likely to be ideal for any given task. Published atlases will probably have too few or too many guide stars, too few or too many deep-sky objects plotted in them, wrong- size charts, etc. I found that with MegaStar I could design and make, specifically for my survey, a “just right” personalized atlas. My atlas consists of 108 charts, each about twenty square degrees in size, with guide stars down to magnitude 8.9. I used only the northernmost 78 charts, since I observed the sky only down to –35°. On the charts I plotted only the objects I wanted to observe. In addition I made enlargements of small, overcrowded areas (“quad charts”) as well as separate large-scale charts for the Virgo Galaxy Cluster, the latter with guide stars down to magnitude 11.4. I put the charts in plastic sheet protectors in a three-ring binder, taking them out and plac- ing them on my telescope mount’s clipboard as needed. To find an object I would use the 35 mm finder (except in the Virgo Cluster, where I used the 60 mm as the finder) to point the ensemble of telescopes at the indicated spot among the guide stars. If the object was not seen in the 35 mm, as it usually was not, I would then look in the larger telescopes. If the object was not immediately visible even in the primary telescope – a not uncommon occur- rence due to inexact initial pointing – I would then scan around for it. -
Evaluation of the National Guideline Clearinghouse (NGC)
Final Report Evaluation of AHRQ’s National Guideline Clearinghouse™ (NGC) Agency for Healthcare Research and Quality August 31, 2011 AFYA, Inc. 8101 Sandy Spring Road, Third Floor Laurel, MD 20707 Final Contract Report: NGC Evaluation Final Submitted: 9/29/2011 Final Contract Report Evaluation of AHRQ’s National Guideline Clearinghouse™ (NGC) Prepared for: Agency for Healthcare Research and Quality U.S. Department of Health and Human Services 540 Gaither Road Rockville, MD 20850 www.ahrq.gov Prepared by: AFYA, Inc. Analytical and Technical Support Division 8101 Sandy Spring Road, Third Floor Laurel, MD 20707 Authors: Michelle Bieber-Tregear AFYA, Inc. Jenice James AFYA, Inc. Debra Dekker AFYA, Inc. Craig Dearfield AFYA, Inc. Jaclyn Marshall Lewin Group Jacob Epstein Lewin Group Carol Simon Lewin Group Financial Declarations None of the authors has any affiliations or financial involvement that conflict with the material presented in this report. Policy Statement This report was prepared by AFYA, Inc. and The Lewin Group under Contract No. 4203; Order No. 3, entitled “Evaluation of the National Guideline Clearinghouse™ (NGC),” with the Department of Health and Human Services’ Agency for Healthcare Research and Quality. Table of Contents List of Figures............................................................................................................................ 5 List of Tables ............................................................................................................................. 6 AHRQ Contract No. 4203; -
WAVES of EXTRATERRESTRIAL ORIGIN DISSERTATION Presented
AN INVESTIGATION AND ANALYSIS OF RATIO ' WAVES OF EXTRATERRESTRIAL ORIGIN DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State University By HSIEN-CHING KO, B.S., M.S. The Ohio State University 1 9 # Approved by: _ Adviser Department of Electrical Engineering ACKNOWLEDGEMENTS The research presented in this dissertation was done at the Radio Observatory of The Ohio State University under the supervision of Professor John D* Kraus who originated the radio astronory project, designed the radio telescope and guided the research. The author wishes to express his sincere appreciation to Professor Kraus, his adviser, for his helpful guidance, discussion and review of the manuscript. For three years he has continuously- provided the author with every assistance possible in order that the present investigation could be successfully completed. Dr. Kraus has contributed many valuable new ideas throughout the investigation* It is a pleasure to acknowledge the work of Mr. Dorm Van Stoutenburg in connection with the improvement and maintenance of the equipment. Thanks are also due many others who participated in the construction of the radio telescope. In addition, rry thanks go to Miss Pi-Yu Chang and Miss Justine Wilson for their assistance in the preparation of the manuscript, and to Mr. Charles E. Machovec of the Physics Library for his cooperation in using the reference materials• The radio astronony project is supported ty grants from the Development Fund, -
Globular Clusters, Though
Appendix: What You’re Looking At Early astronomers divided astronomical objects into three main types: planets, stars, and what were called mists or clouds; in Latin, nebulae. Stars had fixed positions relative to one another, but the planets moved about, and so the ancient Greeks called them wanderers, plan¯et¯es. The changing positions of the planets were hard to explain, and none of the Solar System models proposed bytheancientGreeksorRomansadequatelyexplainedthingssuchasretrograde motion. But even though they didn’t understand why the planets moved about, the Greeks and Romans both placed huge value on interpreting the movements of the planets. This is the art of astrology, a practice that has developed independently in many different cultures around the world. That stars were in some way similar to the Sun was something the ancient Greeks had guessed at, but it wasn’t until the nineteenth century and the invention of spec- troscopy that scientists could demonstrate that the light produced by the Sun was the similar to that produced by the stars. Over time different types of stars were identi- fied, and it soon became clear that the Sun was a relatively small and ordinary star by cosmic standards, even though it is vitally important to us. Nebulae posed particular problems for astronomers prior to the invention of the telescope. To the naked eye all nebulae look alike, nothing more than faint, misty patches of light. Only with the telescope was the diversity of nebulae revealed, but while they could be seen to be morphologically different, astronomers of the early modern era didn’t understand that a planetary nebula is a very different thing to something like the Great Nebula in Andromeda, what we’d today recognize as a galaxy. -
Ngc #21-15 Ngc #21-15 Ngc #21-15
TAH OIL AND GAS CONSERVATION COMMISSIGN REMARKS: WELLLOG ELECTRICLOGs X WATERSANDS LOCATIONINSPECTED SUB. REPORT/abd. DATE FILED LAND:FEE & PATENTED STATELEASENO PUBLICLEASENo U-10760 INDIAN DRILLINGAPPROVED: SPUDDED IN: COMPLETED: PUT TO PRODUCING: IN1TIAL PRODUCTION: GRAVITY A.P.I. GOR: PRODUCINGZONES .. TOTAL DEPTH: WELL ELEVATION: DATEABANDONED: FIELD: Monutilent Butte UNIT: cOUNTY: Duchesne WELLNO. Federal NGC #21-15 API# 43-013-30614 ' LOCATION 660 FT. FROM (N) Å LINE, FT FROM i (W) LINE. NE NN 1/4 - 1/4 SEC Chinle Motas Alluvium Wahweap Shinarump Manning Canyon Lake beds Masuk Moenkopi Mississippian Pleistocene Colorado Sinbad Humbug Lake beds Sego PERMIAN Brazer TERTIARY Buck Tongue Kaibab Pilot Shale Pliocene Castlegate Coconino Madison Salt Lake Mancos Cutler Leadville Oligocene Upper Hoskinnini Redwall Norwood Middle DeChelly DEVONIAN Eocene Lower White Rim Upper Duchesne River Emery Organ Rock Middle Uinta Blue Gate Cedar Mesa Lower Bridger Ferron Halgaite Tongue Ouray Green River Frontier Phosphoria Elbert Dakota Park City McCracken Burro Canyon Rico (Goodridge) Aneth Cedar Mountain Supai Simonson Dolomite Buckhorn Wolfcamp Sevy Dolomite JURASSIC CARBONI FEROUS North Point Wasatch Morrison Pennsylvanian SILURIAN Stone Cabin Salt Wash Oguirrh Laketown Dolomite Colton San Rafeal Gr. Weber ORDOVICIAN Flagstaff Summerville Morgan Eureka Quartzite North Horn Bluff Sandstone Hermosa Pogonip Limestone Almy . Curtis CAMBRIAN Paleocene Entrada Pardox Lynch Current Creek Moab Tongue Ismay Bowman North Horn Carmel Desert Creek Tapeats CRETACEOUS Glen Canyon Gr. Akab Ophir Montana Navajo Barker Creek Tintic Mesaverde Kayenta PRE - CAMBRIAN cekh AS 9 9 NATURAL GAS CORPORATION OF CALIFORNIA 85South2OOEast VernaL Utah 84078 (801)789-4573 September 18, 1981 Mr. E. W. Guynn Geological Survey-Conservation Div. -
A Abell 21, 20–21 Abell 37, 164 Abell 50, 264 Abell 262, 380 Abell 426, 402 Abell 779, 51 Abell 1367, 94 Abell 1656, 147–148
Index A 308, 321, 360, 379, 383, Aquarius Dwarf, 295 Abell 21, 20–21 397, 424, 445 Aquila, 257, 259, 262–264, 266–268, Abell 37, 164 Almach, 382–383, 391 270, 272, 273–274, 279, Abell 50, 264 Alnitak, 447–449 295 Abell 262, 380 Alpha Centauri C, 169 57 Aquila, 279 Abell 426, 402 Alpha Persei Association, Ara, 202, 204, 206, 209, 212, Abell 779, 51 404–405 220–222, 225, 267 Abell 1367, 94 Al Rischa, 381–382, 385 Ariadne’s Hair, 114 Abell 1656, 147–148 Al Sufi, Abdal-Rahman, 356 Arich, 136 Abell 2065, 181 Al Sufi’s Cluster, 271 Aries, 372, 379–381, 383, 392, 398, Abell 2151, 188–189 Al Suhail, 35 406 Abell 3526, 141 Alya, 249, 255, 262 Aristotle, 6 Abell 3716, 297 Andromeda, 327, 337, 339, 345, Arrakis, 212 Achird, 360 354–357, 360, 366, 372, Auriga, 4, 291, 425, 429–430, Acrux, 113, 118, 138 376, 380, 382–383, 388, 434–436, 438–439, 441, Adhara, 7 391 451–452, 454 ADS 5951, 14 Andromeda Galaxy, 8, 109, 140, 157, Avery’s Island, 13 ADS 8573, 120 325, 340, 345, 351, AE Aurigae, 435 354–357, 388 B Aitken, Robert, 14 Antalova 2, 224 Baby Eskimo Nebula, 124 Albino Butterfly Nebula, 29–30 Antares, 187, 192, 194–197 Baby Nebula, 399 Albireo, 70, 269, 271–272, 379 Antennae, 99–100 Barbell Nebula, 376 Alcor, 153 Antlia, 55, 59, 63, 70, 82 Barnard 7, 425 Alfirk, 304, 307–308 Apes, 398 Barnard 29, 430 Algedi, 286 Apple Core Nebula, 280 Barnard 33, 450 Algieba, 64, 67 Apus, 173, 192, 214 Barnard 72, 219 Algol, 395, 399, 402 94 Aquarii, 335 Barnard 86, 233, 241 Algorab, 98, 114, 120, 136 Aquarius, 295, 297–298, 302, 310, Barnard 92, 246 Allen, Richard Hinckley, 5, 120, 136, 320, 324–325, 333–335, Barnard 114, 260 146, 188, 258, 272, 286, 340–341 Barnard 118, 260 M.E. -
X-Ray Emission of Galaxies; Rosat Latest Results
67 X-RAY EMISSION OF GALAXIES; ROSAT LATEST RESULTS Wolfgang Pietsch Max Planck Institut fiir extraterrestrische Physik D-8046 Garching, Federal Rep. of Germany ABSTRACT First results of pointed and All Sky Survey observations of galaxies with the X-ray observatory satellite ROSAT are reported. Survey correlations with IRAS galaxies led to the detection of spiral galaxies with X-ray luminosities of up to 1043 erg s-1 . During observations of the Magellanic Clouds and the Andromeda galaxy new super-soft X-ray sources have been detected. This new class of luminous X-ray sources may help to solve the millisecond pulsar progenitor problem. Due to the improved sensitivity and longer observation times of ROSAT new X-ray point sources have been resolved in several nearby galaxies. The diffuse emission of the LMC that was already reported by EINS TEIN has been been mapped in detail. It shows a lot of fine structure and K. ROSAT temperatures around 5 x 106 The improved low energy response of led to the discovery of 106 K gas from the spiral galaxy MlOl and the halo of the starburst galaxy NGC 253. No diffuseemission was detected from the halo of the edge-on spiral galaxy NGC 5907. 68 W. PIETSCH 1. INTRODUCTION 10 EINSTEIN More than years aftPr t. hP observations with the satellite a com prehensive analysis of normal galaxies is collected in An X-Ray Catalog and Atlaa of Galaziea1) and The X-Ray Spectra of Galazies2),3). The catalog consists of 493 galaxies, 238 of which are detected, for 212 upper limits are given, some are at the edge of the fieldof view or confused with other X-ray sources. -
Discover the Sky's Deepest, Darkest Secrets
On the road with Astronomy were homeowners Adam and Tracy Clay- son. I met them in April 2005 on a tour I led to view the total solar eclipse from the South Pacific. I admit to being envi- ous of their observatory, which houses a Discover the sky’s deepest, 30-inch f/4.5 Obsession reflector. Other notables were friends Jack and Alice Newton and comet-discoverer Stu- darkest secrets art Wilson. Jack Newton is one of the world’s premier astroimagers and a long- Over three dark nights in southern Arizona, two observers track down time contributor to Astronomy. While he dozens of the sky’s most exotic objects. by Michael E. Bakich mainly uses his own impressive observa- tory to hunt for supernovae, Jack and I ’ve been an amateur astronomer for did enjoy one early evening binocular more than 40 years. When I settle hunt of dark nebulae in Aquila. I down to observe the deep sky, I expect Wilson is renowned for his discovery to have a great time. I don’t want weather of Comet 1961V (Wilson-Hubbard). He and lights to be issues. saw it near the star Tau (τ) Geminorum My boss, Astronomy Editor David J. while piloting a Pan American 707 jet Eicher, feels the same. That’s why we from Honolulu to Portland July 23, 1961. traveled to Rancho Hidalgo Astronomy Village in Animas, New Mexico, last If you’re observing in the fall, why not target Developer Eugene Turner (left) poses with The first night October. This site boasts an unbeatable NGC 1, the first object in the New General Cata- Astronomy’s Editor David J. -
Curved Tooth Flexible Gear Couplings
Curved Tooth Flexible Gear Couplings Fenner Curved Tooth Flexible Gear Couplings are the result of many years of experience in the field of Mechanical Power Transmission. These Gear Couplings are distinguished by their mechanical flexibility and compensation of Angular, Parallel and Axial misalignments of the connected shafts. They are made for extensive use in Metal Rolling Mills, Paper Machinery, Cranes, Dredgers, Rubber and Plastic Industries, Cement Plants, Conveyors and Elevators, Compressors, Fans and Blowers, Screens and other general industries. Flexible Gear Couplings basically consist of two hubs, with crowned external teeth and two outer sleeves with internal spur teeth. Gear Hubs and the outer sleeves are manufactured from carbon steel and are hardended to the required degree. They are machined to fine tolerances for proper meshing of the gears as well as for inter-changeability. Curved Tooth Flexible Gear Couplings Curved Tooth Flexible Gear Couplings HUBS : The teeth of Gear Hubs are crowned and are generated POWER RATINGS : by involute system. The amount of crowning and The normal power ratings are given in the Table. For selection of the backlash values are so chosen as to ensure the best correct size of couplings, proper service factor depending on the type results in torque transmission, greater flexibility and of machines and the peak load should be considered. smooth operations. SERVICE FACTOR : SLEEVES : Generally, for medium duty use a service factor of 1.5. For heavy The internal teeth of the sleeves are produced in gear duty use a factor of 2 and for extra heavy duty a factor of 3 should be shaper ensuring the correct profile.