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SAC's 110 Best of the NGC
SAC's 110 Best of the NGC by Paul Dickson Version: 1.4 | March 26, 1997 Copyright °c 1996, by Paul Dickson. All rights reserved If you purchased this book from Paul Dickson directly, please ignore this form. I already have most of this information. Why Should You Register This Book? Please register your copy of this book. I have done two book, SAC's 110 Best of the NGC and the Messier Logbook. In the works for late 1997 is a four volume set for the Herschel 400. q I am a beginner and I bought this book to get start with deep-sky observing. q I am an intermediate observer. I bought this book to observe these objects again. q I am an advance observer. I bought this book to add to my collect and/or re-observe these objects again. The book I'm registering is: q SAC's 110 Best of the NGC q Messier Logbook q I would like to purchase a copy of Herschel 400 book when it becomes available. Club Name: __________________________________________ Your Name: __________________________________________ Address: ____________________________________________ City: __________________ State: ____ Zip Code: _________ Mail this to: or E-mail it to: Paul Dickson 7714 N 36th Ave [email protected] Phoenix, AZ 85051-6401 After Observing the Messier Catalog, Try this Observing List: SAC's 110 Best of the NGC [email protected] http://www.seds.org/pub/info/newsletters/sacnews/html/sac.110.best.ngc.html SAC's 110 Best of the NGC is an observing list of some of the best objects after those in the Messier Catalog. -
X-Ray Luminosities for a Magnitude-Limited Sample of Early-Type Galaxies from the ROSAT All-Sky Survey
Mon. Not. R. Astron. Soc. 302, 209±221 (1999) X-ray luminosities for a magnitude-limited sample of early-type galaxies from the ROSAT All-Sky Survey J. Beuing,1* S. DoÈbereiner,2 H. BoÈhringer2 and R. Bender1 1UniversitaÈts-Sternwarte MuÈnchen, Scheinerstrasse 1, D-81679 MuÈnchen, Germany 2Max-Planck-Institut fuÈr Extraterrestrische Physik, D-85740 Garching bei MuÈnchen, Germany Accepted 1998 August 3. Received 1998 June 1; in original form 1997 December 30 Downloaded from https://academic.oup.com/mnras/article/302/2/209/968033 by guest on 30 September 2021 ABSTRACT For a magnitude-limited optical sample (BT # 13:5 mag) of early-type galaxies, we have derived X-ray luminosities from the ROSATAll-Sky Survey. The results are 101 detections and 192 useful upper limits in the range from 1036 to 1044 erg s1. For most of the galaxies no X-ray data have been available until now. On the basis of this sample with its full sky coverage, we ®nd no galaxy with an unusually low ¯ux from discrete emitters. Below log LB < 9:2L( the X-ray emission is compatible with being entirely due to discrete sources. Above log LB < 11:2L( no galaxy with only discrete emission is found. We further con®rm earlier ®ndings that Lx is strongly correlated with LB. Over the entire data range the slope is found to be 2:23 60:12. We also ®nd a luminosity dependence of this correlation. Below 1 log Lx 40:5 erg s it is consistent with a slope of 1, as expected from discrete emission. -
ARRAKIS: Atlas of Resonance Rings As Known in The
Astronomy & Astrophysics manuscript no. arrakis˙v12 c ESO 2018 September 28, 2018 ARRAKIS: atlas of resonance rings as known in the S4G⋆,⋆⋆ S. Comer´on1,2,3, H. Salo1, E. Laurikainen1,2, J. H. Knapen4,5, R. J. Buta6, M. Herrera-Endoqui1, J. Laine1, B. W. Holwerda7, K. Sheth8, M. W. Regan9, J. L. Hinz10, J. C. Mu˜noz-Mateos11, A. Gil de Paz12, K. Men´endez-Delmestre13 , M. Seibert14, T. Mizusawa8,15, T. Kim8,11,14,16, S. Erroz-Ferrer4,5, D. A. Gadotti10, E. Athanassoula17, A. Bosma17, and L.C.Ho14,18 1 University of Oulu, Astronomy Division, Department of Physics, P.O. Box 3000, FIN-90014, Finland e-mail: [email protected] 2 Finnish Centre of Astronomy with ESO (FINCA), University of Turku, V¨ais¨al¨antie 20, FI-21500, Piikki¨o, Finland 3 Korea Astronomy and Space Science Institute, 776, Daedeokdae-ro, Yuseong-gu, Daejeon 305-348, Republic of Korea 4 Instituto de Astrof´ısica de Canarias, E-38205 La Laguna, Tenerife, Spain 5 Departamento de Astrof´ısica, Universidad de La Laguna, E-38200, La Laguna, Tenerife, Spain 6 Department of Physics and Astronomy, University of Alabama, Box 870324, Tuscaloosa, AL 35487 7 European Space Agency, ESTEC, Keplerlaan 1, 2200 AG, Noorwijk, the Netherlands 8 National Radio Astronomy Observatory/NAASC, 520 Edgemont Road, Charlottesville, VA 22903, USA 9 Space Telescope Science Institute, 3700 San Antonio Drive, Baltimore, MD 21218, USA 10 European Southern Observatory, Casilla 19001, Santiago 19, Chile 11 MMTO, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA 12 Departamento de Astrof´ısica, -
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 -
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. -
Ngc Catalogue Ngc Catalogue
NGC CATALOGUE NGC CATALOGUE 1 NGC CATALOGUE Object # Common Name Type Constellation Magnitude RA Dec NGC 1 - Galaxy Pegasus 12.9 00:07:16 27:42:32 NGC 2 - Galaxy Pegasus 14.2 00:07:17 27:40:43 NGC 3 - Galaxy Pisces 13.3 00:07:17 08:18:05 NGC 4 - Galaxy Pisces 15.8 00:07:24 08:22:26 NGC 5 - Galaxy Andromeda 13.3 00:07:49 35:21:46 NGC 6 NGC 20 Galaxy Andromeda 13.1 00:09:33 33:18:32 NGC 7 - Galaxy Sculptor 13.9 00:08:21 -29:54:59 NGC 8 - Double Star Pegasus - 00:08:45 23:50:19 NGC 9 - Galaxy Pegasus 13.5 00:08:54 23:49:04 NGC 10 - Galaxy Sculptor 12.5 00:08:34 -33:51:28 NGC 11 - Galaxy Andromeda 13.7 00:08:42 37:26:53 NGC 12 - Galaxy Pisces 13.1 00:08:45 04:36:44 NGC 13 - Galaxy Andromeda 13.2 00:08:48 33:25:59 NGC 14 - Galaxy Pegasus 12.1 00:08:46 15:48:57 NGC 15 - Galaxy Pegasus 13.8 00:09:02 21:37:30 NGC 16 - Galaxy Pegasus 12.0 00:09:04 27:43:48 NGC 17 NGC 34 Galaxy Cetus 14.4 00:11:07 -12:06:28 NGC 18 - Double Star Pegasus - 00:09:23 27:43:56 NGC 19 - Galaxy Andromeda 13.3 00:10:41 32:58:58 NGC 20 See NGC 6 Galaxy Andromeda 13.1 00:09:33 33:18:32 NGC 21 NGC 29 Galaxy Andromeda 12.7 00:10:47 33:21:07 NGC 22 - Galaxy Pegasus 13.6 00:09:48 27:49:58 NGC 23 - Galaxy Pegasus 12.0 00:09:53 25:55:26 NGC 24 - Galaxy Sculptor 11.6 00:09:56 -24:57:52 NGC 25 - Galaxy Phoenix 13.0 00:09:59 -57:01:13 NGC 26 - Galaxy Pegasus 12.9 00:10:26 25:49:56 NGC 27 - Galaxy Andromeda 13.5 00:10:33 28:59:49 NGC 28 - Galaxy Phoenix 13.8 00:10:25 -56:59:20 NGC 29 See NGC 21 Galaxy Andromeda 12.7 00:10:47 33:21:07 NGC 30 - Double Star Pegasus - 00:10:51 21:58:39 -
April Night Sky: Galaxy Rankings and Notes
April Night Sky: Galaxy Rankings and Notes Ranking Object Notes M51 Large spiral with connected companion NGC 5195; a must see. M63 “Sunflower galaxy”, bright core, averted vision in larger scope shows mottling. M106 Spiral w/ extended halo; excellent object. NGC 5005 Mottling and extended structure. NGC 4244 Large elongated edge-on galaxy; faint but observable with 8" and larger scopes. NGC 4490 Irregular shape w/ faint companion; should be good target in all scopes. NGC 4449 Irregular w/ visible structure. NGC 4111 Small, bright edge-on galaxy w/ a blue and orange double HJ 2596 to the NE in the same fov. M94 Bright, small core; doesn't display much structure in telescopes. NGC 4631 Irregularly shaped edge-on w/ small faint companion. "The Whale Galaxy" Hook-shaped 4656 just SE. NGC 4565 Large edge-on galaxy w/ dark lane through nucleus; a must see. M64 Excellent object; averted vision in 8" scope shows dark lane thereby the name "Blackeye Galaxy". NGC 4293 Faint, large edgewise galaxy; challenge in smaller instruments. NGC 4450 Face on spiral; faint but displays structure in large scope. M85 Excellent target w/ visible neighbor galaxy in same fov. M100 Low surface brightness but very large; hint of spiral structure w/ averted vision. NGC 4216 Bright core w/ faint extended arms; nearly edgewise spiral. M98 Excellent object w/ nearby star to the NE with structure visible near nucleus. M99 Difficult to discern much structure; shows some irregularity in shape. Markarian’s Chain Several galaxies in a sweeping arc beginning with M84 and M86 and sweeping NE; a must see in large binoculars and all telescopes. -
The ACS Virgo Cluster Survey. VI. Isophotal Analysis and Surface Brightness Profiles 3 at Odds with Previous Claims in Lauer Et Al
Rochester Institute of Technology RIT Scholar Works Articles 2006 The CA S Virgo Cluster Survey. VI. Isophotal Analysis and the Structure of Early-Type Galaxies Laura Ferrarese National Research Council of Canada Patrick Côté National Research Council of Canada Andrés Jordán European Southern Observatory Eric W. Peng National Research Council of Canada John P. Blakeslee The Johns Hopkins University See next page for additional authors Follow this and additional works at: http://scholarworks.rit.edu/article Recommended Citation Laura Ferrarese et al 2006 ApJS 164 334 https://doi.org/10.1086/501350 This Article is brought to you for free and open access by RIT Scholar Works. It has been accepted for inclusion in Articles by an authorized administrator of RIT Scholar Works. For more information, please contact [email protected]. Authors Laura Ferrarese, Patrick Côté, Andrés Jordán, Eric W. Peng, John P. Blakeslee, Slawomir Piatek, Simona Mei, David Merritt, Miloš Milosavljević, John L. Tonry, and Michael J. West This article is available at RIT Scholar Works: http://scholarworks.rit.edu/article/1182 Accepted by The Astrophysical Journal Supplements Preprint typeset using LATEX style emulateapj v. 10/10/03 THE ACS VIRGO CLUSTER SURVEY. VI. ISOPHOTAL ANALYSIS AND THE STRUCTURE OF EARLY-TYPE GALAXIES1 Laura Ferrarese2, Patrick Cotˆ e´2, Andres´ Jordan´ 3,4, Eric W. Peng2, John P. Blakeslee5,6, Slawomir Piatek7, Simona Mei5, David Merritt8, Miloˇs Milosavljevic´9,10, John L. Tonry11, & Michael J. West12 Accepted by The Astrophysical Journal Supplements ABSTRACT We present a detailed analysis of the morphology, isophotal parameters and surface brightness profiles for 100 early-type members of the Virgo Cluster, from dwarfs (MB = −15.1 mag) to giants (MB = −21.8 mag). -
Binocular Universe
Binocular Universe: A Few Hairy Objects April 2014 Phil Harrington lear skies come few and far between at this time of year, at least in my neck of the C woods, so I like to take advantage of just about every one that happens along. The old saying that April showers bring May flowers is alive and well here in the northeastern U.S., as this is traditionally one of the cloudiest and wettest months of the year. Above: Spring star map from Star Watch by Phil Harrington. Asterism Above: Finder chart for this month's Binocular Universe . Chart adapted from Touring the Universe through Binoculars Atlas (TUBA), www.philharrington.net/tuba.htm One of the reasons I'm so keen to observe the April sky is the Coma Berenices Star Cluster , one of my favorite binocular targets. It’s one of those objects that does nothing through telescopes, but really comes alive through binoculars. That’s because the star cluster spans more than 7.5 degrees of sky. To find it, aim toward the center of the large, "empty" area framed by the constellations Boötes to the east, Leo to the west, and the arc of the Big Dipper's handle to the north. Scan back and forth slowly until you bump into a wedge-shaped group of stars that will likely fill the field of your binoculars. That's the Coma Star Cluster. In fact, if you are viewing from a dark site, you can see the Coma Star Cluster as a fuzzy patch of light without using any optical aid at all. -
Southern Sentinel Observing Session Notes
Southern Sentinel Observing Session Notes Observing Session - Thursday 24th April 2003 Date: 24 Apr 2002 (Local) Time: 2145-2345 NZDT (UT +12) Location: Pauanui, Coromandel Peninsula. 120 Minutes From Home. Weather: Clear, Mild and Calm conditions. Seeing: Limiting Magnitude 5.5, transparency 3.5/5, seeing 3/5 Moon: No Moon (Small Waxing Moon, Set) Equipment: 13.1" F5 Dob with Paracorr, TeleVue Eyepieces, UHC Filter After a break of three weeks this time, Michelle and I planned a long weekend at Pauanui with the inclusion of Anzac Day. The weather looked to be pretty good and was liked to be settled for the whole weekend. Arriving from Auckland at 9 PM at Pauanui, I was observing 45 minutes later after the obligatory unpacking and settling in. The conditions were mild and clear. The skies were dark and through the gap in the large pines a dark Northeast aspect presented a good chance to work at the Virgo Cluster again. There was no dew all night and the seeing was average to good. The plan for the whole weekend was the systematic logging of the whole Virgo Coma Berenices region. This would start tonight from Vindemiatrix past Rho Virginis. Objects seen were; Object Type Altitude Magnification Eyepiece ------ ---- -------- ------------- -------- NGC 4689 Galaxy 36.2° 114x TeleVue 17mm Nagler Type 4 NGC 4762 Galaxy 38.6° 114x TeleVue 17mm Nagler Type 4 NGC 4754 Galaxy 38.5° 114x TeleVue 17mm Nagler Type 4 NGC 4880 Galaxy 36.8° 114x TeleVue 17mm Nagler Type 4 NGC 4866 Galaxy 35.5° 114x TeleVue 17mm Nagler Type 4 NGC 4654 Galaxy 38.1° 114x -
Binocular Certificate Handbook
Irish Federation of Astronomical Societies Binocular Certificate Handbook How to see 110 extraordinary celestial sights with an ordinary pair of binoculars © John Flannery, South Dublin Astronomical Society, August 2004 No ordinary binoculars! This photograph by the author is of the delightfully whimsical frontage of the Chiat/Day advertising agency building on Main Street, Venice, California. Binocular Certificate Handbook page 1 IFAS — www.irishastronomy.org Introduction HETHER NEW to the hobby or advanced am- Wateur astronomer you probably already own Binocular Certificate Handbook a pair of a binoculars, the ideal instrument to casu- ally explore the wonders of the Universe at any time. Name _____________________________ Address _____________________________ The handbook you hold in your hands is an intro- duction to the realm far beyond the Solar System — _____________________________ what amateur astronomers call the “deep sky”. This is the abode of galaxies, nebulae, and stars in many _____________________________ guises. It is here that we set sail from Earth and are Telephone _____________________________ transported across many light years of space to the wonderful and the exotic; dense glowing clouds of E-mail _____________________________ gas where new suns are being born, star-studded sec- tions of the Milky Way, and the ghostly light of far- Observing beginner/intermediate/advanced flung galaxies — all are within the grasp of an ordi- experience (please circle one of the above) nary pair of binoculars. Equipment __________________________________ True, the fixed magnification of (most) binocu- IFAS club __________________________________ lars will not allow you get the detail provided by telescopes but their wide field of view is perfect for NOTES: Details will be treated in strictest confidence. -
RASC Finest NGC Observing Program Checklist
RASC Finest NGC Observing Program Checklist Use this checklist to monitor your progress. Version 1.0a. Edited on 9 June 2021. Record your detailed observations on the provided observing forms or your own log sheets. Sketching is optional but highly encouraged. The "+" column denotes special combination objects. E.g. FNGC # 26 is for NGC 1973 with 1975 and 1977. Number NGC + Alternate ID Con Cls RA 2000 Decl 2000 Mag Size Rating Done The Autumn Sky 1 NGC 7009 Saturn Nebula Aqr PN 21h04m10.9s -11°21'48" 8.3 28" !! q 2 NGC 7293 Helix Aqr PN 22h29m38.5s -20°50'14" 6.3 16.0' !! q 3 NGC 7331 Deer Lick Group Peg Gal 22h37m04.3s +34°24'59" 10.2 9.1'x 3.4' !! q 4 NGC 7635 Bubble Nebula Cas EN 23h20m43.0s +61°12'31" 11 16.0'x 9.0' q 5 NGC 7789 OCL 269 Cas OC 23h57m24.0s +56°42'30" 7.5 25.0' !! q 6 NGC 185 MCG 8-2-10 Cas Gal 00h38m57.9s +48°20'15" 10.2 10.7'x 8.9' q 7 NGC 281 PacMan Nebula Cas EN 00h53m00.0s +56°37'00" 7.4 30.0' !! q 8 NGC 457 ET Cluster Cas OC 01h19m35.0s +58°17'12" 5.1 20.0' q 9 NGC 663 Collinder 20 Cas OC 01h46m09.0s +61°14'06" 6.4 14.0' q 10 IC 289 PN G138.8+02.8 Cas PN 03h10m19.3s +61°19'01" 12 45" q 11 NGC 7662 Blue Snowball And PN 23h25m54.0s +42°32'05" 8.6 17" !! q 12 NGC 891 Silver Needle And Gal 02h22m33.6s +42°20'46" 10.9 11.7'x 2.3' !! q 13 NGC 253 Sculptor Galaxy Scl Gal 00h47m33.1s -25°17'20" 7.9 28.2'x 5.5' !! q 14 NGC 772 Arp 78 Ari Gal 01h59m20.0s +19°00'28" 10.6 5.9'x 3.2' q 15 NGC 246 Skull Nebula Cet PN 00h47m03.3s -11°52'19" 10.4 4.0' q 16 NGC 936 MCG 0-7-17 Cet Gal 02h27m37.5s -01°09'20" 11.2 4.5'x 3.4' q 17