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The Desert Sky Observer
Desert Sky Observer Volume 32 Antelope Valley Astronomy Club Newsletter February 2012 Up-Coming Events February 10: Club Meeting* February 11: Moon Walk @ Prime Desert Woodlands February 13: Executive Board Meeting @ Don’s house February 18: Telescope Night and Star Party @ Devil's Punchbowl * Monthly meetings are held at the S.A.G.E. Planetarium on the Cactus School campus in Palmdale, the second Friday of each month. The meeting location is at the northeast corner of Avenue R and 20th Street East. Meetings start at 7 p.m. and are open to the public. Please note that food and drink are not allowed in the planetarium President Don Bryden Well I gave a star party and no one showed up! Not that I can blame them – it was raining and windy and cold – it even hailed! Still I dragged out the scope and got it ready to go. Briefly, between the clouds I looked at Jupiter and it was quite a treat. The Galilean moons were all tight to the planet either coming from just in front or behind. It gave a bejeweled look like a large ruby surrounded by four small diamonds. Even with the winds and clouds the sky was surprisingly steady and I went as high as 260x with ease, exposing the shadow of Europa transiting the planet. But soon more clouds came and inside we had a nice fire so I put the Artist's rendering DVD “400 Years of the Telescope” on and settled in for the night. My daughter had a few friends over after a skating party that afternoon and later when I went out for one more look they came out to see what was up. -
Arxiv:0804.4630V1 [Astro-Ph] 29 Apr 2008 I Ehnv20;Ficao 06) Ti Nti Oeas Role This in Is It 2006A)
DRAFT VERSION NOVEMBER 9, 2018 Preprint typeset using LATEX style emulateapj v. 05/04/06 OPEN CLUSTERS AS GALACTIC DISK TRACERS: I. PROJECT MOTIVATION, CLUSTER MEMBERSHIP AND BULK THREE-DIMENSIONAL KINEMATICS PETER M. FRINCHABOY1,2,3 AND STEVEN R. MAJEWSKI2 Department of Astronomy, University of Virginia, P.O. Box 400325, Charlottesville, VA 22904-4325, USA Draft version November 9, 2018 ABSTRACT We have begun a survey of the chemical and dynamical properties of the Milky Way disk as traced by open star clusters. In this first contribution, the general goals of our survey are outlined and the strengths and limita- tions of using star clusters as a Galactic disk tracer sample are discussed. We also present medium resolution (R 15,0000) spectroscopy of open cluster stars obtained with the Hydra multi-object spectrographs on the Cerro∼ Tololo Inter-American Observatory 4-m and WIYN 3.5-m telescopes. Here we use these data to deter- mine the radial velocities of 3436 stars in the fields of open clusters within about 3 kpc, with specific attention to stars having proper motions in the Tycho-2 catalog. Additional radial velocity members (without Tycho-2 proper motions) that can be used for future studies of these clusters were also identified. The radial velocities, proper motions, and the angular distance of the stars from cluster center are used to derive cluster member- ship probabilities for stars in each cluster field using a non-parametric approach, and the cluster members so-identified are used, in turn, to derive the reliable bulk three-dimensional motion for 66 of 71 targeted open clusters. -
The Ara Ob1a Association: Stellar Population and Star Formation History
Astronomy & Astrophysics manuscript no. 15497 c ESO 2018 November 7, 2018 The Ara OB1a association Stellar population and star formation history G. Baume1,⋆, G. Carraro2,⋆⋆, F. Comeron3, and G. C. de El´ıa1 1 Facultad de Ciencias Astron´omicas y Geof´ısicas (UNLP), Instituto de Astrof´ısica de La Plata (CONICET, UNLP), Paseo del Bosque s/n, La Plata, Argentina e-mail: [email protected] e-mail: [email protected] 2 ESO, Alonso de Cordova 3107, Vitacura, Santiago de Chile, Chile e-mail: [email protected] 3 ESO, Karl-Schwarzschild-Strasse 2 85748 Garching bei Munchen Germany e-mail: [email protected] Received: June 10, 2010; Accepted: April 26, 2011 ABSTRACT Context. The Ara OB1a association is a nearby complex in the fourth Galactic quadrant where a number of young/embedded star clusters are projected close to more evolved, intermediate age clusters. It is also rich in interstellar matter, and contains evidence of the interplay between massive stars and their surrounding medium, such as the rim HII region NGC 6188. Aims. We provide robust estimates of the fundamental parameters (age and distance) of the two most prominent stellar clusters, NGC 6167 and NGC 6193, that may be used as a basis for studing the star formation history of the region. Methods. The study is based on a photometric optical survey (UBVIHα) of NGC 6167 and NGC 6193 and their nearby field, complemented with public data from 2MASS-VVV, UCAC3, and IRAC-Spitzer in this region. Results. We produce a uniform photometric catalogue and estimate more robustly the fundamental parameters of NGC 6167 and NGC 6193, in addition to the IRAS 16375-4854 source. -
Proto-Planetary Nebula Observing Guide
Proto-Planetary Nebula Observing Guide www.reinervogel.net RA Dec CRL 618 Westbrook Nebula 04h 42m 53.6s +36° 06' 53" PK 166-6 1 HD 44179 Red Rectangle 06h 19m 58.2s -10° 38' 14" V777 Mon OH 231.8+4.2 Rotten Egg N. 07h 42m 16.8s -14° 42' 52" Calabash N. IRAS 09371+1212 Frosty Leo 09h 39m 53.6s +11° 58' 54" CW Leonis Peanut Nebula 09h 47m 57.4s +13° 16' 44" Carbon Star with dust shell M 2-9 Butterfly Nebula 17h 05m 38.1s -10° 08' 33" PK 10+18 2 IRAS 17150-3224 Cotton Candy Nebula 17h 18m 20.0s -32° 27' 20" Hen 3-1475 Garden-sprinkler Nebula 17h 45m 14. 2s -17° 56' 47" IRAS 17423-1755 IRAS 17441-2411 Silkworm Nebula 17h 47m 13.5s -24° 12' 51" IRAS 18059-3211 Gomez' Hamburger 18h 09m 13.3s -32° 10' 48" MWC 922 Red Square Nebula 18h 21m 15s -13° 01' 27" IRAS 19024+0044 19h 05m 02.1s +00° 48' 50.9" M 1-92 Footprint Nebula 19h 36m 18.9s +29° 32' 50" Minkowski's Footprint IRAS 20068+4051 20h 08m 38.5s +41° 00' 37" CRL 2688 Egg Nebula 21h 02m 18.8s +36° 41' 38" PK 80-6 1 IRAS 22036+5306 22h 05m 30.3s +53° 21' 32.8" IRAS 23166+1655 23h 19m 12.6s +17° 11' 33.1" Southern Objects ESO 172-7 Boomerang Nebula 12h 44m 45.4s -54° 31' 11" Centaurus bipolar nebula PN G340.3-03.2 Water Lily Nebula 17h 03m 10.1s -47° 00' 27" PK 340-03 1 IRAS 17163-3907 Fried Egg Nebula 17h 19m 49.3s -39° 10' 37.9" Finder charts measure 20° (with 5° circle) and 5° (with 1° circle) and were made with Cartes du Ciel by Patrick Chevalley (http://www.ap-i.net/skychart) Images are DSS Images (blue plates, POSS II or SERCJ) and measure 30’ by 30’ (http://archive.stsci.edu/cgi- bin/dss_plate_finder) and STScI Images (Hubble Space Telescope) Downloaded from www.reinervogel.net version 12/2012 DSS images copyright notice: The Digitized Sky Survey was produced at the Space Telescope Science Institute under U.S. -
Atlas Menor Was Objects to Slowly Change Over Time
C h a r t Atlas Charts s O b by j Objects e c t Constellation s Objects by Number 64 Objects by Type 71 Objects by Name 76 Messier Objects 78 Caldwell Objects 81 Orion & Stars by Name 84 Lepus, circa , Brightest Stars 86 1720 , Closest Stars 87 Mythology 88 Bimonthly Sky Charts 92 Meteor Showers 105 Sun, Moon and Planets 106 Observing Considerations 113 Expanded Glossary 115 Th e 88 Constellations, plus 126 Chart Reference BACK PAGE Introduction he night sky was charted by western civilization a few thou - N 1,370 deep sky objects and 360 double stars (two stars—one sands years ago to bring order to the random splatter of stars, often orbits the other) plotted with observing information for T and in the hopes, as a piece of the puzzle, to help “understand” every object. the forces of nature. The stars and their constellations were imbued with N Inclusion of many “famous” celestial objects, even though the beliefs of those times, which have become mythology. they are beyond the reach of a 6 to 8-inch diameter telescope. The oldest known celestial atlas is in the book, Almagest , by N Expanded glossary to define and/or explain terms and Claudius Ptolemy, a Greco-Egyptian with Roman citizenship who lived concepts. in Alexandria from 90 to 160 AD. The Almagest is the earliest surviving astronomical treatise—a 600-page tome. The star charts are in tabular N Black stars on a white background, a preferred format for star form, by constellation, and the locations of the stars are described by charts. -
Astronomy Astrophysics
A&A 412, 431–445 (2003) Astronomy DOI: 10.1051/0004-6361:20031455 & c ESO 2003 Astrophysics A 12CO (J =1 0) study towards the Ara OB1 region ! E. M. Arnal1;2;?,J.May3, and G. A. Romero1;?? 1 Instituto Argentino de Radioastronom´ıa (IAR), C.C. No. 5, 1894 Villa Elisa, Argentina 2 Facultad de Ciencias Astron´omicas y Geof´ısica Universidad Nacional de La Plata, Paseo del Bosque s/n, 1900 La Plata, Argentina 3 Departamento de Astronom´ıa, Universidad de Chile, Casilla 36-D, Santiago, Chile Received 19 May 2003 / Accepted 8 September 2003 12 Abstract. Intermediate angular resolution (HPBW = 8:07) carbon monoxide ( CO J = 1 0) line observations towards the → OB association Ara OB1 are reported. The molecular line observations cover an area of 2◦:75 3◦:00, and disclose a rich and complex distribution of the molecular line emission. The molecular features likely to be associated× with the OB-association 1 Ara OB1 span the velocity range from 28 to 20 km s− . The most negative radial velocities are observed along NGC 6188 ( Rim nebula). This nebula marks the interface− − between the Hii region RCW 108 and the highly absorbing molecular material located≡ westwards of the ionised region. The dominant CO structures, labeled E and F, have a radial velocity of about 23:5 1 − and 21:8kms− , respectively. The former harbours a bright optical knot, the infrared cluster RCW-108 and the strong IRAS source− 16362 4845. IRAS point sources are also seen in projection onto 12CO concentrations F and H. This may indicate that the star forming− process is a widespread phenomenon in this molecular complex. -
Astronomy & Astrophysics Two Highly Reddened Young
A&A 388, 179–188 (2002) Astronomy DOI: 10.1051/0004-6361:20020540 & c ESO 2002 Astrophysics Two highly reddened young open clusters located beyond the Sagittarius arm?,?? A. E. Piatti1 and J. J. Clari´a2 1 Instituto de Astronom´ıa y F´ısica del Espacio, CC 67, Suc. 28, 1428, Buenos Aires, Argentina 2 Observatorio Astron´omico, Universidad Nacional de C´ordoba, Laprida 854, 5000 C´ordoba, Argentina Received 10 October 2001 / Accepted 3 April 2002 Abstract. We present the results of CCD BV I Johnson-Cousins photometry down to V ∼ 19 mag in the regions of the unstudied stellar groups Pismis 23 and BH 222, both projected close to the direction towards the Galactic centre. We measured V magnitude and B − V and V − I colours for a total of 928 stars in fields of about 40×40. Pismis 23 is conclusively a physical system, since a clear main sequence and other meaningful features can be seen in the colour-magnitude diagrams. The reality of this cluster is also supported by star counts carried out within and outside the cluster field. For Pismis 23 we derive colour excesses E(B−V )=2.0 0.1andE(V −I)=2.6 0.1, a distance from the Sun of 2.6 0.6kpc(Z = −19 pc) and an age of 300 100 Myr (assuming solar metal content). BH 222 appears to be a young open cluster formed by a vertical main sequence and by a conspicuous group of luminous, typically red supergiant stars. We derived for this cluster a colour excess of E(V −I)=2.4 0.2, a distance from the Sun of 6.0 2.7kpc(Z = −46 pc) and an age of 60 30 Myr. -
Southern Sky Binocular Observing List
Southern Sky Binocular Observing List Object R.A. DEC Mag PA* Type Size Const Urn SA [ ] NGC 104 00 24.1 -72 05 4.5 ----- GbCl 25.0' Tuc 440 24 [ ] SMC 00 52.8 -72 50 2.7 10 Glxy 316'X186' Tuc 441 24 [ ] NGC 362 01 03.2 -70 51 6.6 ----- GbCl 12.9' Tuc 441 24 [ ] NGC 1261 03 12.3 -55 13 8.4 ----- GbCl 6.9' Hor 419 24 [ ] NGC 1851 05 14.1 -40 03 7.2 ----- GbCl 11.0' Col 393 19 [ ] LMC 05 23.6 -69 45 0.9 170 Glxy 646'X550' Dor 444 24 [ ] NGC 2070 05 38.6 -69 05 8.2 ----- BNeb 40'X25' Dor 445 24 [ ] NGC 2451 07 45.4 -37 58 2.8 ----- OpCl 45.0' Pup 362 19 [ ] NGC 2477 07 52.3 -38 33 5.8 ----- OpCl 27.0' Pup 362 19 [ ] NGC 2516 07 58.3 -60 52 3.8 ----- OpCl 29.0' Car 424 24 [ ] NGC 2547 08 10.7 -49 16 4.7 ----- OpCl 20.0' Vel 396 20 [ ] NGC 2546 08 12.4 -37 38 6.3 ----- OpCl 40.0' Pup 362 20 [ ] NGC 2627 08 37.3 -29 57 8.4 ----- OpCl 11.0' Pyx 363 20 [ ] IC 2391 08 40.2 -53 04 2.5 ----- OpCl 50.0' Vel 425 25 [ ] IC 2395 08 41.1 -48 12 4.6 ----- OpCl 7.0' Vel 397 20 [ ] NGC 2659 08 42.6 -44 57 8.6 ----- OpCl 2.7' Vel 397 20 [ ] NGC 2670 08 45.5 -48 47 7.8 ----- OpCl 9.0' Vel 397 20 [ ] NGC 2808 09 12.0 -64 52 6.3 ----- GbCl 13.8' Car 448 25 [ ] IC 2488 09 27.6 -56 59 7.4 ----- OpCl 14.0' Vel 425 25 [ ] NGC 2910 09 30.4 -52 54 7.2 ----- OpCl 5.0' Vel 426 25 [ ] NGC 2925 09 33.7 -53 26 8.3 ----- OpCl 12.0' Vel 426 25 [ ] NGC 3114 10 02.7 -60 07 4.2 ----- OpCl 35.0' Car 426 25 [ ] NGC 3201 10 17.6 -46 25 6.7 ----- GbCl 18.0' Vel 399 20 [ ] NGC 3228 10 21.8 -51 43 6.0 ----- OpCl 18.0' Vel 426 25 [ ] NGC 3293 10 35.8 -58 14 4.7 ----- OpCl 5.0' Car -
Allcharts2018-08.Pdf
The Evening Sky in August 2018 Four naked-eye planets are visible in the early evening sky. Three of them are the brightest 'stars' in the sky. Silver Venus appears midway down the northwest sky soon after sunset. Golden Jupiter is north of the zenith and orange Mars is midway up the eastern sky. As the sky darkens Saturn appears roughly midway between Jupiter and Mars, more toward Mars as the month progresses. It is fainter than Jupiter and Mars but still the brightest 'star' in its part of the sky. Bright stars are widely scattered. Vega on the north skyline is balanced by Canopus low in the south. Orange Arcturus is in the northwest. The Southern Cross, Crux, and the Pointers are midway down the southwest sky. The Milky Way spans the sky from northeast to southwest. Venus sets due west more than three hours after the sun, making it a spectacular object in a dark sky. It is bright enough to see by naked eye during the day if you can focus on infinity. At noon Venus is level with the Sun and 46 degrees east (right) of the Sun. That's a bit more than two hand-spans at arm's length. It is best to be in the shade to try this sighting. In a telescope Venus looks like a first-quarter Moon. The Moon is near Venus on the 14th and 15th, near Jupiter on the 17th and 18th, close to Saturn on the 21st, and passing by Mars on the 23rd and 24th. At the beginning of August Mars is the closest it has been since 2003, 58 million km from us. -
Skytools Chart
36 Ara - Pavo SkyTools 3 / Skyhound.com 2 ζ 6541 NGC 6231 ζ NGC 6124 θ NGC 6322 η η 6496 ζ 1 6388 PK 345-04.1 -4 NGC 6259 NGC 6192 0° 1 ε NGC 6249 ι 1 δ α PK 342-04.1 β IC 4699 μ σ Mu Normae Cluster β2 NGC 6250 NGC 6178 NGC 6204 6352 ω NGC 6200 δ ζ λ θ α IC 4651 NGC 6193 ε ι PK 342-14.1 NGC 6134 6584 6326 NGC 6167 2 Ara γ η 6397 γ1 λ ε1 NGC 6152 α NGC 6208 1 ν μ β 5946 γ ζ NGC 6067 -50° ξ PK 331-05.1 κ 5927 PK 329-02.2 η ζ η NGC 6087 NGC 5999 NGC 5925 Pavo Globular δ 6221 ι1 ξ Collinder 292 α NGC 5822 ν λ 6300 NGC 5823 NGC 6025 π NGC 5749 6744 η PK 325-12.1 γ β β φ1 Pavo δ β NGC 5662 ρ 6362 κ ζ Circinus δ Triangulum Australe ε α Rigel Kentaurus ε 5844 2 -6 α 0 ° β NGC 5617 ζ ζ α Agena 6101 γ γ NGC 5316 ε Apus PK 315-13.1 -7 0° NGC 5281 2 1h h 5 52° x 34° 1 18h 18h00m00.0s -60°00'00" (Skymark) Globular Cl. Dark Neb. Galaxy 8 7 6 5 4 3 2 1 Globule Planetary Open Cl. Nebula 36 Ara - Pavo GALASSIE Sigla Nome Cost. A.R. Dec. Mv. Dim. Tipo Distanza 200/4 80/11,5 20x60 NGC 6221 Ara 16h 52m 47s -59° 12' 59" +10,70 4',6x2',8 Sc 18,0 Mly --- --- --- NGC 6300 Ara 17h 16m 59s -62° 49' 11" +11,00 5',5x3',5 SBb 34,0 Mly --- --- --- NGC 6744 Pav 19h 09m 46s -63° 51' 28" +9,10 17',0x10',7 SABb 21,0 Mly --- --- --- AMMASSI APERTI Sigla Nome Cost. -
South Binoculars
South Binoculars (66 objects) Object Type Mag Size Information 47 Tucanae GC 4.0 50.0' R00:24:05.2 D-72:04:49 Tucana NGC 104 Type: III NGC 362 GC 6.8 14.0' R01:03:14.3 D-70:50:52 Tucana Type: III NGC 1261 GC 8.3 6.8' R03:12:15.3 D-55:12:59 Horologium Type: II NGC 1851 GC 7.1 12.0' R05:14:06.3 D-40:02:48 Columba Type: II Tarantula Nebula BN 30.0'x20.0' R05:38:42.5 D-69:06:03 Dorado NGC 2070 Type: EN, mag_b: 5.0 NGC 2451 OC 2.8 50.0' R07:45:15.0 D-37:58:00 Puppis Type: II2p NGC 2477 OC 5.8 20.0' R07:52:10.0 D-38:31:48 Puppis Type: I3r NGC 2516 OC 3.8 22.0' R07:58:04.0 D-60:45:12 Carina Type: I3r, mag_b: 3.8 NGC 2547 OC 4.7 25.0' R08:10:09.0 D-49:12:54 Vela Type: II2p NGC 2546 OC 6.3 70.0' R08:12:15.0 D-37:35:42 Puppis Type: III2m NGC 2627 OC 8.4 9.0' R08:37:15.0 D-29:57:18 Pyxis Type: III2m Omicron Velorum OC 2.6 60.0' R08:40:18.0 D-52:55:00 Vela cluster Type: II3p IC 2391 IC 2395 OC 4.6 13.0' R08:42:30.0 D-48:08:12 Vela Type: II3p NGC 2659 OC 8.6 15.0' R08:42:36.0 D-44:59:00 Vela Type: III3m NGC 2670 OC 7.8 7.0' R08:45:30.0 D-48:48:00 Vela Type: II2p NGC 2808 GC 6.2 14.0' R09:12:02.6 D-64:51:45 Carina Type: I IC 2488 OC 7.4 18.0' R09:27:31.0 D-56:58:54 Vela Type: II2m NGC 2910 OC 7.2 6.0' R09:30:29.0 D-52:54:50 Vela Type: I2p NGC 3114 OC 4.2 35.0' R10:02:36.0 D-60:07:00 Carina Type: II3r 1/4 South Binoculars (66 objects) Object Type Mag Size Information NGC 3201 GC 6.9 20.0' R10:17:36.8 D-46:24:38 Vela Type: X NGC 3228 OC 6.0 5.0' R10:21:22.0 D-51:43:42 Vela Type: I1p Gem Cluster OC 4.7 5.0' R10:35:51.0 D-58:13:48 Carina NGC 3293 Type: -
Jack Bennett's Catalogue of Southern Comet-Like Deep-Sky Objects
Jack Bennett’s Catalogue of Southern Comet-like Deep-sky Objects Deep-sky Observing Challenge Compiled by Auke Slotegraaf Director: ASSA Deep-Sky Observing Section. Version 4.2, November 2013 Jack Bennett and his catalogue For two decades, starting in the late 1960’s, the southern sky was patrolled by a dedicated South African comet-hunter named Jack Bennett. He observed from his urban backyard with a 5-inch low-power refractor. Not only did he discover two comets, he also picked up a 9th magnitude supernova in NGC 5236 (M83), becoming the first person ever to visually discover a supernova since the invention of the telescope. Bennett was born on April 6th, 1914 and passed away on May 30th, 1990. A long-standing member of the Astronomical Society of Southern Africa (ASSA), he was elected President in 1969. The Society awarded him the prestigious Gill Medal for services to astronomy in 1970 and in 1986 he received an Honorary Degree of Master of Science from the University of Witwatersrand. In 1989, at the recommendation of Rob McNaught of Siding Springs Observatory, the asteroid VD 4093 was named after him. Bennett was a skilled observer and in the spirit of Charles Messier drew up two lists of southern objects that appeared comet-like in his telescope. His first list (Bennett, 1969) was published four months before he discovered his first comet. The supplementary list (Bennett, 1974) was followed three months later by his second discovery. In his 1969 Presidential Address to the ASSA Bennett said: “As an aid to the recognition of comet-like objects in the Southern sky, and to help observers to eliminate them in comet searches, I have over the past five years compiled a list of 130 such objects visible south of the celestial equator.