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Arxiv:1911.09125V2 [Astro-Ph.SR] 23 Jun 2020 Maccarone Et Al
Draft version June 25, 2020 Typeset using LATEX twocolumn style in AASTeX63 A Dynamical Survey of Stellar-Mass Black Holes in 50 Milky Way Globular Clusters Newlin C. Weatherford,1, 2 Sourav Chatterjee,3 Kyle Kremer,1, 2 Frederic A. Rasio,1, 2 1Department of Physics & Astronomy, Northwestern University, Evanston, IL 60208, USA 2Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, IL 60208, USA 3Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India ABSTRACT Recent numerical simulations of globular clusters (GCs) have shown that stellar-mass black holes (BHs) play a fundamental role in driving cluster evolution and shaping their present-day structure. Rapidly mass-segregating to the center of GCs, BHs act as a dynamical energy source via repeated super-elastic scattering, delaying onset of core collapse and limiting mass segregation for visible stars. While recent discoveries of BH candidates in Galactic and extragalactic GCs have further piqued inter- est in BH-mediated cluster dynamics, numerical models show that even if significant BH populations remain in today's GCs, they are not typically in directly detectable configurations. We demonstrated in Weatherford et al.(2018) that an anti-correlation between a suitable measure of mass segregation (∆) in observable stellar populations and the number of retained BHs in GC models can be applied to indirectly probe BH populations in real GCs. Here, we estimate the number and total mass of BHs in 50 Milky Way GCs from the ACS Globular Cluster Survey. For each GC, ∆ is measured between observed main sequence populations and fed into correlations between ∆ and BH retention found in our CMC Cluster Catalog's models. -
Study of the Existence of Active Galactic Nuclei of the Evolution and Disappearance of the Torus Through X-Rays
Universidad Nacional Autónoma de México Instituto de Radioastronomía y Astrofísica PhD. in Science (Astrophysics) Advance of doctoral project Study of the existence of Active Galactic Nuclei of the evolution and disappearance of the torus through X-rays PRESENTS: Natalia Osorio Clavijo ADVISOR: Dra. Omaira González Martín June 2021 1 Introduction It has been widely accepted that all galaxies with developed bulges, host a super massive black hole (SMBH), which in some cases is being fed by an accretion disk, causing the liberation of energy of orders up to bolometric luminosities L ∼ 1044 erg s−1. The nuclei of galaxies with such phenomenon are known as active galactic nuclei (AGN), and can emit through all the electromagnetic spectrum. According to the standard model (Urry and Padovani, 1995) AGN are composed by several regions apart from the accretion disk. Such regions are made up from clouds of dust and gas, although their formation and evolution are still under debate. Among the components, we find the SMBH, whose mass can be of the 6 10 order of ∼ 10 − 10 M , the accretion disk, which is responsible for the accretion onto the SMBH and most of the energy released. The temperature of this structure places the peak of emission at opti- cal/UV wavelengths. The broad line region (BLR) is placed beyond the accretion disk and is formed by clouds of gas, with speeds of several thousands of km/s (Davidson and Netzer, 1979), producing the broadening of lines emitted in the optical and infrarred range (e.g., Hα,Hβ, the Paschen series, etc.) This region is surrounded by the torus, a region composed by dust that is heated by the accretion disk up to a few 1000 of K, placing the peak of its emission at infrared wavelengths. -
Mining SDSS in Search of Multiple Populations in Globular Clusters
A&A 525, A114 (2011) Astronomy DOI: 10.1051/0004-6361/201015662 & c ESO 2010 Astrophysics Mining SDSS in search of multiple populations in globular clusters C. Lardo1, M. Bellazzini2, E. Pancino2, E. Carretta2, A. Bragaglia2, and E. Dalessandro1 1 Department of Astronomy, University of Bologna, via Ranzani 1, 40127 Bologna, Italy e-mail: [email protected] 2 INAF - Osservatorio Astronomico di Bologna, via Ranzani 1, 40127 Bologna, Italy Received 31 August 2010 / Accepted 6 October 2010 ABSTRACT Several recent studies have reported the detection of an anomalous color spread along the red giant branch (RGB) of some globular clusters (GC) that appears only when color indices including a near ultraviolet band (such as Johnson U or Strömgren u) are con- sidered. This anomalous spread in color indexes such as U − B or cy has been shown to correlate with variations in the abundances of light elements such as C, N, O, Na, etc., which, in turn, are generally believed to be associated with subsequent star formation episodes that occurred in the earliest few 108 yr of the cluster’s life. Here we use publicly available u, g, r Sloan Digital Sky Survey photometry to search for anomalous u − g spreads in the RGBs of nine Galactic GCs. In seven of them (M 2, M 3, M 5, M 13, M 15, M 92 and M 53), we find evidence of a statistically significant spread in the u − g color, not seen in g − r and not accounted for by observational effects. In the case of M 5, we demonstrate that the observed u − g color spread correlates with the observed abundances of Na, the redder stars being richer in Na than the bluer ones. -
SPIRIT Target Lists
JANUARY and FEBRUARY deep sky objects JANUARY FEBRUARY OBJECT RA (2000) DECL (2000) OBJECT RA (2000) DECL (2000) Category 1 (west of meridian) Category 1 (west of meridian) NGC 1532 04h 12m 04s -32° 52' 23" NGC 1792 05h 05m 14s -37° 58' 47" NGC 1566 04h 20m 00s -54° 56' 18" NGC 1532 04h 12m 04s -32° 52' 23" NGC 1546 04h 14m 37s -56° 03' 37" NGC 1672 04h 45m 43s -59° 14' 52" NGC 1313 03h 18m 16s -66° 29' 43" NGC 1313 03h 18m 15s -66° 29' 51" NGC 1365 03h 33m 37s -36° 08' 27" NGC 1566 04h 20m 01s -54° 56' 14" NGC 1097 02h 46m 19s -30° 16' 32" NGC 1546 04h 14m 37s -56° 03' 37" NGC 1232 03h 09m 45s -20° 34' 45" NGC 1433 03h 42m 01s -47° 13' 19" NGC 1068 02h 42m 40s -00° 00' 48" NGC 1792 05h 05m 14s -37° 58' 47" NGC 300 00h 54m 54s -37° 40' 57" NGC 2217 06h 21m 40s -27° 14' 03" Category 1 (east of meridian) Category 1 (east of meridian) NGC 1637 04h 41m 28s -02° 51' 28" NGC 2442 07h 36m 24s -69° 31' 50" NGC 1808 05h 07m 42s -37° 30' 48" NGC 2280 06h 44m 49s -27° 38' 20" NGC 1792 05h 05m 14s -37° 58' 47" NGC 2292 06h 47m 39s -26° 44' 47" NGC 1617 04h 31m 40s -54° 36' 07" NGC 2325 07h 02m 40s -28° 41' 52" NGC 1672 04h 45m 43s -59° 14' 52" NGC 3059 09h 50m 08s -73° 55' 17" NGC 1964 05h 33m 22s -21° 56' 43" NGC 2559 08h 17m 06s -27° 27' 25" NGC 2196 06h 12m 10s -21° 48' 22" NGC 2566 08h 18m 46s -25° 30' 02" NGC 2217 06h 21m 40s -27° 14' 03" NGC 2613 08h 33m 23s -22° 58' 22" NGC 2442 07h 36m 20s -69° 31' 29" Category 2 Category 2 M 42 05h 35m 17s -05° 23' 25" M 42 05h 35m 17s -05° 23' 25" NGC 2070 05h 38m 38s -69° 05' 39" NGC 2070 05h 38m 38s -69° -
The Hubble Catalog of Variables (HCV)? A
Astronomy & Astrophysics manuscript no. hcv c ESO 2019 September 25, 2019 The Hubble Catalog of Variables (HCV)? A. Z. Bonanos1, M. Yang1, K. V. Sokolovsky1; 2; 3, P. Gavras4; 1, D. Hatzidimitriou1; 5, I. Bellas-Velidis1, G. Kakaletris6, D. J. Lennon7; 8, A. Nota9, R. L. White9, B. C. Whitmore9, K. A. Anastasiou5, M. Arévalo4, C. Arviset8, D. Baines10, T. Budavari11, V. Charmandaris12; 13; 1, C. Chatzichristodoulou5, E. Dimas5, J. Durán4, I. Georgantopoulos1, A. Karampelas14; 1, N. Laskaris15; 6, S. Lianou1, A. Livanis5, S. Lubow9, G. Manouras5, M. I. Moretti16; 1, E. Paraskeva1; 5, E. Pouliasis1; 5, A. Rest9; 11, J. Salgado10, P. Sonnentrucker9, Z. T. Spetsieri1; 5, P. Taylor9, and K. Tsinganos5; 1 1 IAASARS, National Observatory of Athens, Penteli 15236, Greece e-mail: [email protected] 2 Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA 3 Sternberg Astronomical Institute, Moscow State University, Universitetskii pr. 13, 119992 Moscow, Russia 4 RHEA Group for ESA-ESAC, Villanueva de la Cañada, 28692 Madrid, Spain 5 Department of Physics, National and Kapodistrian University of Athens, Panepistimiopolis, Zografos 15784, Greece 6 Athena Research and Innovation Center, Marousi 15125, Greece 7 Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain 8 ESA, European Space Astronomy Centre, Villanueva de la Canada, 28692 Madrid, Spain 9 Space Telescope Science Institute, Baltimore, MD 21218, USA 10 Quasar Science Resources for ESA-ESAC, Villanueva de la Cañada, 28692 Madrid, Spain 11 The Johns Hopkins University, Baltimore, MD 21218, USA 12 Institute of Astrophysics, FORTH, Heraklion 71110, Greece 13 Department of Physics, Univ. -
Caldwell Catalogue - Wikipedia, the Free Encyclopedia
Caldwell catalogue - Wikipedia, the free encyclopedia Log in / create account Article Discussion Read Edit View history Caldwell catalogue From Wikipedia, the free encyclopedia Main page Contents The Caldwell Catalogue is an astronomical catalog of 109 bright star clusters, nebulae, and galaxies for observation by amateur astronomers. The list was compiled Featured content by Sir Patrick Caldwell-Moore, better known as Patrick Moore, as a complement to the Messier Catalogue. Current events The Messier Catalogue is used frequently by amateur astronomers as a list of interesting deep-sky objects for observations, but Moore noted that the list did not include Random article many of the sky's brightest deep-sky objects, including the Hyades, the Double Cluster (NGC 869 and NGC 884), and NGC 253. Moreover, Moore observed that the Donate to Wikipedia Messier Catalogue, which was compiled based on observations in the Northern Hemisphere, excluded bright deep-sky objects visible in the Southern Hemisphere such [1][2] Interaction as Omega Centauri, Centaurus A, the Jewel Box, and 47 Tucanae. He quickly compiled a list of 109 objects (to match the number of objects in the Messier [3] Help Catalogue) and published it in Sky & Telescope in December 1995. About Wikipedia Since its publication, the catalogue has grown in popularity and usage within the amateur astronomical community. Small compilation errors in the original 1995 version Community portal of the list have since been corrected. Unusually, Moore used one of his surnames to name the list, and the catalogue adopts "C" numbers to rename objects with more Recent changes common designations.[4] Contact Wikipedia As stated above, the list was compiled from objects already identified by professional astronomers and commonly observed by amateur astronomers. -
Nuclear Activity in Circumnuclear Ring Galaxies
International Journal of Astronomy and Astrophysics, 2016, 6, 219-235 Published Online September 2016 in SciRes. http://www.scirp.org/journal/ijaa http://dx.doi.org/10.4236/ijaa.2016.63018 Nuclear Activity in Circumnuclear Ring Galaxies María P. Agüero1, Rubén J. Díaz2,3, Horacio Dottori4 1Observatorio Astronómico de Córdoba, UNCand CONICET, Córdoba, Argentina 2ICATE, CONICET, San Juan, Argentina 3Gemini Observatory, La Serena, Chile 4Instituto de Física, UFRGS, Porto Alegre, Brazil Received 23 May 2016; accepted 26 July 2016; published 29 July 2016 Copyright © 2016 by authors and Scientific Research Publishing Inc. This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/ Abstract We have analyzed the frequency and properties of the nuclear activity in a sample of galaxies with circumnuclear rings and spirals (CNRs), compiled from published data. From the properties of this sample a typical circumnuclear ring can be characterized as having a median radius of 0.7 kpc (mean 0.8 kpc, rms 0.4 kpc), located at a spiral Sa/Sb galaxy (75% of the hosts), with a bar (44% weak, 37% strong bars). The sample includes 73 emission line rings, 12 dust rings and 9 stellar rings. The sample was compared with a carefully matched control sample of galaxies with very similar global properties but without detected circumnuclear rings. We discuss the relevance of the results in regard to the AGN feeding processes and present the following results: 1) bright companion galaxies seem -
The Astrophysical Journal Supplement Series, 45:259-334
.259W The Astrophysical Journal Supplement Series, 45:259-334, 1981 February 45. © 1981. The American Astronomical Society. All rights reserved. Printed in U.S.A. ... 198lApJS A CATALOG OF RADIAL VELOCITIES IN GALACTIC GLOBULAR CLUSTERS1 R. F. Webbink Department of Astronomy, University of Illinois at Urbana-Champaign Received 1980 February 25; accepted 1980 July 9 ABSTRACT A catalog of all stellar and integrated radial velocities of galactic globular clusters published prior to 1980 is assembled here. Known systematic errors in the data are discussed, and data on 686 stars and 85 globular clusters are presented in the body of the catalog; an Appendix lists published radial velocities in 4 dwarf spheroidal satellites of the Galaxy. Weighted mean velocities for each of the 89 systems in the catalog and Appendix are calculated. Subject headings: clusters: globular— stars: catalogs I. INTRODUCTION data. No catalog of individual stellar and cluster veloci- Radial velocities of galactic globular clusters were ties exists as such. first obtained in the pioneering surveys by Slipher (1918, The present catalog is intended to fill the need for a 1919, 1922, 1924), at Lowell Observatory, and by San- comprehensive listing of all available globular cluster ford (1918, 1919a,6), at Mount Wilson, who together radial velocity data and to provide a systematic reassess- obtained velocities of 18 clusters. In the more than 60 ment of the cluster velocities on this basis. To the best of years since those studies, several other radial velocity the author’s knowledge, all data published prior to 1980 surveys have been published, of which the most exten- January 1 are included here. -
Optical Astronomy Observatories
National Optical Astronomy Observatories National Optical Astronomy Observatories Quarterly Report July - September 1989 TABLE OF CONTENTS I. INTRODUCTION j II. SCIENTIFIC HIGHLIGHTS 2 A. Ages of Globular Ousters 2 B. Disk Galaxies in Formation 2 C. Differential Rotation Observed in the Sun as a Star 3 D. Intensity Oscillations in the Far-Infrared 4 E. Supergranular Convection 4 F. Brown Dwarfs: A Detection of Stellar Objects of Subcritical Mass? 5 G. Cooling Flows in Clusters of Galaxies: Where Are All the Stars? 5 III. PERSONNEL 7 A. Visiting Scientists 7 B. New Appointees 7 C. Terminations 7 D. Change of Status ' g E. Summer Research Assistants 8 IV. INSTRUMENTATION, NEW PROJECTS, AND OBSERVATORY ACTIVITIES .... 9 A. Future Telescope Technology Program (FTT) 9 B. Global Oscillation Network Group (GONG) 9 C. Instrumentation Projects ]\ D. Observatory Activities 16 V. PROGRAM SUPPORT !9 A. Director's Office 19 B. Central Administrative Services 20 C. Central Computer Services 20 D. Central Facilities Operations 20 E. Engineering and Technical Services 21 F. Publications and Information Resources 21 Appendices Appendix A: Telescope Usage Statistics Appendix B: Observational Programs I. INTRODUCTION This quarterly report covers scientific highlights for the period of July - September 1989, as well as personnel changes for the period. These highlights emphasize concluded projects rather than work in progress. The report also discusses new technology for telescopes and instrumentation, GONG, instrumentation projects, and observatory activities. The Engineering and Technical Services division now submits reports for the instrumentation projects, with contributions from program scientists, if necessary. The Associate Directors for CTIO and NSO continue to provide the information of efforts at La Serena/Cerro Tololo and Sacramento Peak. -
108 Afocal Procedure, 105 Age of Globular Clusters, 25, 28–29 O
Index Index Achromats, 70, 73, 79 Apochromats (APO), 70, Averted vision Adhafera, 44 73, 79 technique, 96, 98, Adobe Photoshop Aquarius, 43, 99 112 (software), 108 Aquila, 10, 36, 45, 65 Afocal procedure, 105 Arches cluster, 23 B1620-26, 37 Age Archinal, Brent, 63, 64, Barkhatova (Bar) of globular clusters, 89, 195 catalogue, 196 25, 28–29 Arcturus, 43 Barlow lens, 78–79, 110 of open clusters, Aricebo radio telescope, Barnard’s Galaxy, 49 15–16 33 Basel (Bas) catalogue, 196 of star complexes, 41 Aries, 45 Bayer classification of stellar associations, Arp 2, 51 system, 93 39, 41–42 Arp catalogue, 197 Be16, 63 of the universe, 28 Arp-Madore (AM)-1, 33 Beehive Cluster, 13, 60, Aldebaran, 43 Arp-Madore (AM)-2, 148 Alessi, 22, 61 48, 65 Bergeron 1, 22 Alessi catalogue, 196 Arp-Madore (AM) Bergeron, J., 22 Algenubi, 44 catalogue, 197 Berkeley 11, 124f, 125 Algieba, 44 Asterisms, 43–45, Berkeley 17, 15 Algol (Demon Star), 65, 94 Berkeley 19, 130 21 Astronomy (magazine), Berkeley 29, 18 Alnilam, 5–6 89 Berkeley 42, 171–173 Alnitak, 5–6 Astronomy Now Berkeley (Be) catalogue, Alpha Centauri, 25 (magazine), 89 196 Alpha Orionis, 93 Astrophotography, 94, Beta Pictoris, 42 Alpha Persei, 40 101, 102–103 Beta Piscium, 44 Altair, 44 Astroplanner (software), Betelgeuse, 93 Alterf, 44 90 Big Bang, 5, 29 Altitude-Azimuth Astro-Snap (software), Big Dipper, 19, 43 (Alt-Az) mount, 107 Binary millisecond 75–76 AstroStack (software), pulsars, 30 Andromeda Galaxy, 36, 108 Binary stars, 8, 52 39, 41, 48, 52, 61 AstroVideo (software), in globular clusters, ANR 1947 -
The Caldwell Catalogue+Photos
The Caldwell Catalogue was compiled in 1995 by Sir Patrick Moore. He has said he started it for fun because he had some spare time after finishing writing up his latest observations of Mars. He looked at some nebulae, including the ones Charles Messier had not listed in his catalogue. Messier was only interested in listing those objects which he thought could be confused for the comets, he also only listed objects viewable from where he observed from in the Northern hemisphere. Moore's catalogue extends into the Southern hemisphere. Having completed it in a few hours, he sent it off to the Sky & Telescope magazine thinking it would amuse them. They published it in December 1995. Since then, the list has grown in popularity and use throughout the amateur astronomy community. Obviously Moore couldn't use 'M' as a prefix for the objects, so seeing as his surname is actually Caldwell-Moore he used C, and thus also known as the Caldwell catalogue. http://www.12dstring.me.uk/caldwelllistform.php Caldwell NGC Type Distance Apparent Picture Number Number Magnitude C1 NGC 188 Open Cluster 4.8 kly +8.1 C2 NGC 40 Planetary Nebula 3.5 kly +11.4 C3 NGC 4236 Galaxy 7000 kly +9.7 C4 NGC 7023 Open Cluster 1.4 kly +7.0 C5 NGC 0 Galaxy 13000 kly +9.2 C6 NGC 6543 Planetary Nebula 3 kly +8.1 C7 NGC 2403 Galaxy 14000 kly +8.4 C8 NGC 559 Open Cluster 3.7 kly +9.5 C9 NGC 0 Nebula 2.8 kly +0.0 C10 NGC 663 Open Cluster 7.2 kly +7.1 C11 NGC 7635 Nebula 7.1 kly +11.0 C12 NGC 6946 Galaxy 18000 kly +8.9 C13 NGC 457 Open Cluster 9 kly +6.4 C14 NGC 869 Open Cluster -
190 Index of Names
Index of names Ancora Leonis 389 NGC 3664, Arp 005 Andriscus Centauri 879 IC 3290 Anemodes Ceti 85 NGC 0864 Name CMG Identification Angelica Canum Venaticorum 659 NGC 5377 Accola Leonis 367 NGC 3489 Angulatus Ursae Majoris 247 NGC 2654 Acer Leonis 411 NGC 3832 Angulosus Virginis 450 NGC 4123, Mrk 1466 Acritobrachius Camelopardalis 833 IC 0356, Arp 213 Angusticlavia Ceti 102 NGC 1032 Actenista Apodis 891 IC 4633 Anomalus Piscis 804 NGC 7603, Arp 092, Mrk 0530 Actuosus Arietis 95 NGC 0972 Ansatus Antliae 303 NGC 3084 Aculeatus Canum Venaticorum 460 NGC 4183 Antarctica Mensae 865 IC 2051 Aculeus Piscium 9 NGC 0100 Antenna Australis Corvi 437 NGC 4039, Caldwell 61, Antennae, Arp 244 Acutifolium Canum Venaticorum 650 NGC 5297 Antenna Borealis Corvi 436 NGC 4038, Caldwell 60, Antennae, Arp 244 Adelus Ursae Majoris 668 NGC 5473 Anthemodes Cassiopeiae 34 NGC 0278 Adversus Comae Berenices 484 NGC 4298 Anticampe Centauri 550 NGC 4622 Aeluropus Lyncis 231 NGC 2445, Arp 143 Antirrhopus Virginis 532 NGC 4550 Aeola Canum Venaticorum 469 NGC 4220 Anulifera Carinae 226 NGC 2381 Aequanimus Draconis 705 NGC 5905 Anulus Grahamianus Volantis 955 ESO 034-IG011, AM0644-741, Graham's Ring Aequilibrata Eridani 122 NGC 1172 Aphenges Virginis 654 NGC 5334, IC 4338 Affinis Canum Venaticorum 449 NGC 4111 Apostrophus Fornac 159 NGC 1406 Agiton Aquarii 812 NGC 7721 Aquilops Gruis 911 IC 5267 Aglaea Comae Berenices 489 NGC 4314 Araneosus Camelopardalis 223 NGC 2336 Agrius Virginis 975 MCG -01-30-033, Arp 248, Wild's Triplet Aratrum Leonis 323 NGC 3239, Arp 263 Ahenea