Quarterly Bainbridge Island, WA June 4 Partial Lunar Eclipse (Max 4:12 A.M
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Webfooted Astronomer Seattle Astronomical Society • September 2003 Sept
the Webfooted Astronomer Seattle Astronomical Society • September 2003 Sept. Meeting: September Meeting Galaxy Formation in Speaker: Vandana Desai Rich Clusters Galaxy Formation Vandana Desai grew up in Chicago, in Rich Clusters majored in Astronomy at Caltech in Pasadena, CA, then came directly to Wednesday, September 17 graduate school at the UW, where 7:30 p.m. she is working with Professor Physics-Astronomy Building Julianne Dalcanton. Ms. Desai is Room A102 interested in all topics related to University of Washington galaxy formation and evolution, but Seattle has concentrated her efforts on how galaxies evolve in clusters. Come early at 7 p.m. for coffee and snacks and to visit with your In order to understand this evolu- fellow members! tion, Ms. Desai uses both space- based imaging data as well as numerical simulations. She’ll show examples of both during her talk in September about galaxy formation in rich clusters. She will give a basic description of how galaxies are expected to form if the mass of the Uni- verse is dominated by Cold Dark Matter, and will then discuss how the evolution of a galaxy is affected by its environment, focusing on clusters of galaxies. These are active areas of research at the University of Washing- ton, so she will show us some work in progress, including an extremely high-resolution numerical simulation of galaxies forming within a cluster and new Hubble Space Telescope images of clusters at high redshift. Seattle Astronomical Society Address: Web Page: PO Box 31746 http://seattleastro.org Seattle, -
Martian Ice How One Neutrino Changed Astrophysics Remembering Two Former League Presidents
Published by the Astronomical League Vol. 71, No. 3 June 2019 MARTIAN ICE HOW ONE NEUTRINO 7.20.69 CHANGED ASTROPHYSICS 5YEARS REMEMBERING TWO APOLLO 11 FORMER LEAGUE PRESIDENTS ONOMY T STR O T A H G E N P I E G O Contents N P I L R E B 4 . President’s Corner ASTRONOMY DAY Join a Tour This Year! 4 . All Things Astronomical 6 . Full Steam Ahead OCTOBER 5, From 37,000 feet above the Pacific Total Eclipse Flight: Chile 7 . Night Sky Network 2019 Ocean, you’ll be high above any clouds, July 2, 2019 For a FREE 76-page Astronomy seeing up to 3¼ minutes of totality in a PAGE 4 9 . Wanderers in the Neighborhood dark sky that makes the Sun’s corona look Day Handbook full of ideas and incredibly dramatic. Our flight will de- 10 . Deep Sky Objects suggestions, go to: part from and return to Santiago, Chile. skyandtelescope.com/2019eclipseflight www.astroleague.org Click 12 . International Dark-Sky Association on "Astronomy Day” Scroll 14 . Fire & Ice: How One Neutrino down to "Free Astronomy Day African Stargazing Safari Join astronomer Stephen James ̃̃̃Changed a Field Handbook" O’Meara in wildlife-rich Botswana July 29–August 4, 2019 for evening stargazing and daytime PAGE 14 18 . Remembering Two Former For more information, contact: safari drives at three luxury field ̃̃̃Astronomical League Presidents Gary Tomlinson camps. Only 16 spaces available! Astronomy Day Coordinator Optional extension to Victoria Falls. 21 . Coming Events [email protected] skyandtelescope.com/botswana2019 22 . Gallery—Moon Shots 25 . Observing Awards Iceland Aurorae September 26–October 2, 2019 26 . -
The Leo-I Group: New Dwarf Galaxy and UDG Candidates Oliver Müller1, Helmut Jerjen2, and Bruno Binggeli1
Astronomy & Astrophysics manuscript no. aanda c ESO 2018 February 26, 2018 The Leo-I group: new dwarf galaxy and UDG candidates Oliver Müller1, Helmut Jerjen2, and Bruno Binggeli1 1 Departement Physik, Universität Basel, Klingelbergstr. 82, CH-4056 Basel, Switzerland e-mail: [email protected] 2 Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia Received XX, 2018; accepted TBD ABSTRACT Context. The study of dwarf galaxies and their environments provides crucial testbeds for predictions of cosmological models and insights on the structure formation on small cosmological scales. In recent years, many problems on the scale of groups of galaxies challenged the current standard model of cosmology. Aims. We aim to increase the sample of known galaxies in the Leo-I group, containing the M 96 subgroup and the Leo Triplet. This galaxy aggregate is located at the edge of the Local Volume at a mean distance of 10.7 Mpc. Methods. We employ image enhancing techniques to search for low-surface brightness objects in publicly available gr images taken by the Sloan Digital Sky Survey within 500 square degrees around the Leo-I group. Once detected, we perform surface photometry and compare their structural parameters to other known dwarf galaxies in the nearby universe. Results. We found 36 new dwarf galaxy candidates within the search area. Their morphology and structural parameters resemble known dwarfs in other groups. Among the candidates 5 to 6 galaxies are considered as ultra diffuse galaxies candidates. If confirmed, they would be some of the closest examples of this galaxy type. -
Prime Focus (02-11)
Highlights of the February Sky. - - - 1st - - - DAWN: Use binoculars to Prime Focus find Mercury 3° below a thin crescent Moon 15 A Publication of the Kalamazoo Astronomical Society minutes before sunrise. - - - 2nd - - - February 2011 New Moon 9:31 pm EST - - - 4th - - - AM: Venus is between open clusters M21 & M23. ThisThis MonthsMonths KAS EventsEvents - - - 6th - - - PM: Jupiter is 6.5° to left General Meeting: Friday, February 4 @ 7:00 pm of the Waxing Crescent Moon. Kalamazoo Area Math & Science Center - See Page 14 for Details PM: Uranus is 6° to lower left of the Moon Observing Session: Saturday, February 5 @ 7:00 pm - - - 9th - - - February Freeze Out - Kalamazoo Nature Center AM: The asteroid Vesta (7.8 magnitude) is 0.4° above Venus. Full Moon Theater: Saturday, February 19 @ 7:00 pm WMU Main Campus, Rood Hall, Room 1110 - See Page 3 for Details - - - 11th - - - First Quarter Moon 2:18 am EST AM: Venus is between star clusters M22 & M25. InsideInside thethe Newsletter.Newsletter. .. .. PM: The Moon is about 2° south of the Pleiades. January Meeting Minutes....................... p. 2 - - - 18th - - - Full Moon Board Meeting Minutes......................... p. 2 3:36 am EST Full Moon Theater Preview................. p. 3 - - - 20th - - - Possible Field Trips in 2011................. p. 3 AM: Spica, Saturn, and the gibbous Moon form a KAS Retrospective................................. p. 4 nearly equilateral triangle. Seventy-Five Years of Looking Up......p. 6 - - - 24th - - - A.L. Observing Clubs............................. p. 9 Last Quarter Moon 6:26 pm EST Star Parties in 2011................................ p. 10 - - - 25th - - - NASA Space Place.................................. p. 11 AM: The Moon is about 3° February Night Sky.................................p. -
EAS BUSINESS… Him Know If Plans Change
1 Volume MMXVIII No. 1 January 2018 President: Mark Folkerts folkerts at seanet.com The Stargazer VP and Programs: Ron Mosher ron.mosher69 at gmail.net P.O. Box 13272 Treasurer: Roger Meisner Mill Creek, WA 98082 Web assistance: Mark Folkerts Newsletter co-editors Mark Simonson, Mark Folkerts marknilse at yahoo.com Intro Astro Classes Jack Barnes jackdanielb at comcast.net See EAS website at: Star party organizer Ron Tam tam1951 at frontier.net http://everettastro.org so needs to contact him in advance and confirm available dates, and let EAS BUSINESS… him know if plans change. “Our place is open for star parties any Saturday except weekends of the Full Moon. People can call to get weather conditions or to confirm that there is a star party. Our TH FEB EAS MEETING – SATURDAY FEBRUARY 10 , 3:00 PM, phone number is (360) 568-5152. They can e-mail me too AT EVERGREEN BRANCH LIBRARY, MEETING ROOM ([email protected]) but I don't check my email daily. They can email me for directions if they never have been out here.” The next EAS monthly meeting will be 3:00 pm Call Ron about unscheduled spur-of-the-moment observing. We try Saturday Feb 10th. There will be a video presentation. to hold informal close-in star parties each month during the spring, summer, and fall months on a weekend near the New moon at a member’s property or a local park. EAS meetings have speakers or presentations, and updates on calendar events and upcoming activities, and are open to the Western US Star Parties in 2018 public at no charge. -
MESSIER 15 RA(2000) : 21H 29M 58S DEC(2000): +12° 10'
MESSIER 15 RA(2000) : 21h 29m 58s DEC(2000): +12° 10’ 01” BASIC INFORMATION OBJECT TYPE: Globular Cluster CONSTELLATION: Pegasus BEST VIEW: Late October DISCOVERY: Jean-Dominique Maraldi, 1746 DISTANCE: 33,600 ly DIAMETER: 175 ly APPARENT MAGNITUDE: +6.2 APPARENT DIMENSIONS: 18’ FOV:Starry 1.00Night FOV: 60.00 Vulpecula Sagitta Pegasus NGC 7009 (THE SATURN NEBULA) Delphinus NGC 7009 RA(2000) : 21h 04m 10.8s DEC(2000): -11° 21’ 48.6” Equuleus Pisces Aquila NGC 7009 FOV: 5.00 Aquarius Telrad Capricornus Sagittarius Cetus Piscis Austrinus NGC 7009 Microscopium BASIC INFORMATION OBJECT TYPE: Planetary Nebula CONSTELLATION: Aquarius Sculptor BEST VIEW: Early November DISCOVERY: William Herschel, 1782 DISTANCE: 2000 - 4000 ly DIAMETER: 0.4 - 0.8 ly Grus APPARENT MAGNITUDE: +8.0 APPARENT DIMENSIONS: 41” x 35” Telescopium Telrad Indus NGC 7662 (THE BLUE SNOWBALL) RA(2000) : 23h 25m 53.6s DEC(2000): +42° 32’ 06” BASIC INFORMATION OBJECT TYPE: Planetary Nebula CONSTELLATION: Andromeda BEST VIEW: Late November DISCOVERY: William Herschel, 1784 DISTANCE: 1800 – 6400 ly DIAMETER: 0.3 – 1.1 ly APPARENT MAGNITUDE: +8.6 APPARENT DIMENSIONS: 37” MESSIER 52 RA(2000) : 23h 24m 48s DEC(2000): +61° 35’ 36” BASIC INFORMATION OBJECT TYPE: Open Cluster CONSTELLATION: Cassiopeia BEST VIEW: December DISCOVERY: Charles Messier, 1774 DISTANCE: ~5000 ly DIAMETER: 19 ly APPARENT MAGNITUDE: +7.3 APPARENT DIMENSIONS: 13’ AGE: 50 million years FOV:Starry 1.00Night FOV: 60.00 Auriga Cepheus Andromeda MESSIER 31 (THE ANDROMEDA GALAXY) M 31 RA(2000) : 00h 42m 44.3Cassiopeias DEC(2000): +41° 16’ 07.5” Perseus Lacerta AndromedaM 31 FOV: 5.00 Telrad Triangulum Taurus Orion Aries Andromeda M 31 Pegasus Pisces BASIC INFORMATION OBJECT TYPE: Galaxy CONSTELLATION: Andromeda Telrad BEST VIEW: December DISCOVERY: Abd al-Rahman al-Sufi, 964 Eridanus CetusDISTANCE: 2.5 million ly DIAMETER: ~250,000 ly* APPARENT MAGNITUDE: +3.4 APPARENT DIMENSIONS: 178’ x 63’ (3° x 1°) *This value represents the total diameter of the disk, based on multi-wavelength measurements. -
Existence and Importance of Magnetic Fields in Tight Pairs and Groups of Galaxies 15 3 Summary of the Published Articles 17 3.1
EXISTENCEANDIMPORTANCEOFMAGNETICFIELDSIN TIGHTPAIRSANDGROUPSOFGALAXIES błazej˙ nikiel-wroczynski´ A PhD thesis written under the supervision of Professor Marek Urbanik and co-supervision of Doctor Marek Jamrozy Astronomical Observatory Faculty of Physics, Astronomy and Applied Computer Science Jagiellonian University June 2015 Błazej˙ Nikiel-Wroczy´nski: Existence and importance of magnetic fields in tight pairs and groups of galaxies, © June 2015 supervisors: Prof. dr hab. Marek Urbanik Dr Marek Jamrozy alma mater: Jagiellonian University, Faculty of Physics, Astronomy and Applied Computer Science Dedication This work is dedicated to Rugia for being (probably unknowingly) an Earth-based analogue of the MHD dynamo, that amplified my determination to collect all the presented articles into one thesis, transferring the kinetic energy of my turbulent movements into a genuinely regular (not just anisotropic), scientific dissertation. ABSTRACT This dissertation is an attempt to investigate the existence and role of the intergalactic magnetic fields in compact groups and tight pairs of galaxies. Radio emission from several, well known objects of these types is analysed and properties of the discovered intergalactic mag- netised structures are discussed. Together, these results are used to show that wherever found, intergalactic magnetic fields play impor- tant role in the galactic dynamics and evolution. Non-thermal, in- tergalactic radio emission, which signifies existence of the magnetic fields, can be used as a very sensitive tracer of interactions and gas flows. Unusual magnetised objects and structures can be found in the intergalactic space, and their studies open a possibility to discover more about the cosmic magnetism itself. v PUBLICATIONS This dissertation has been written as a summary of the scientific ac- tivities previously reported in these articles: • Nikiel-Wroczy ´nski,B., Jamrozy, M., Soida, M., Urbanik, M., Multiwavelength study of the radio emission from a tight galaxy pair Arp 143, 2014, MNRAS, 444, 1729 • Nikiel-Wroczy ´nski,B., Soida, M., Bomans, D. -
Oregon Star Party News
OREGON STAR PARTY NEWS Oregon Star Party Newsletter— Volume 3, Issue 2 Late July 2017 How to Maximize Your Time Under Totality By Judy Dethloff For many of you, this total solar eclipse may be a “Once in a Lifetime Opportunity”. While the entire eclipse from first contact to fourth contact is 2 hours 35 minutes, the total phase lasts 1 minute 28 seconds at Indian Trail Spring. Wow, 88 seconds is short! The morning of the eclipse, you are not going to have a second chance for a “Do Over”. How can you maximize your chances for successfully viewing and photographing totality? To fully maximize those precious 88 seconds, you need to have a game plan. Your game plan is going to tell you what time you need to have all of your equipment setup, which pieces of equipment you are using and how you will set it up. Your game plan will tell you Eclipse Times what specific eclipse features you are looking for and the time to look for them. You will First Contact 9:07:17.9 am have decided when to take off and replace your solar filters. Your game plan can be very simple or very complex depending upon how you intend to observe the solar eclipse. You Second Contact 10:21:05.1 am do have a game plan, don’t you? Max Eclipse 10:21:46.9 am Now that you have a game plan, you need to practice it at home to see if it works. Re- member, “Practice makes perfect.” Find something around you that normally takes 90 Third Contact 10:22:28.8 am seconds or so and during that 90 seconds of time visualize what you would do during the total phase. -
Radio Continuum Observations of the Leo Triplet at 2.64
Astronomy & Astrophysics manuscript no. leo264-9 c ESO 2018 June 15, 2018 Radio continuum observations of the Leo Triplet at 2.64 GHz∗ B. Nikiel-Wroczy´nski1, M. Soida1, M. Urbanik1, M. We˙zgowiec2, R. Beck3, D. J. Bomans2,4, and B. Adebahr2 1 Obserwatorium Astronomiczne Uniwersytetu Jagiello´nskiego, ul. Orla 171, 30-244 Krak´ow, Poland 2 Astronomisches Institut, Ruhr-Universit¨at Bochum, Universit¨atsstrasse 150, 44780 Bochum, Germany 3 Max-Planck-Institut f¨ur Radioastronomie, Auf dem H¨ugel 69, 53121 Bonn, Germany 4 Research Department “Plasmas with Complex Interactions”, Ruhr-Universit¨at Bochum, Universit¨atsstrasse 150, 44780 Bochum, Germany Received 11 January 2013/ Accepted 15 March 2013 ABSTRACT Context. The Leo Triplet group of galaxies is best known for the impressive bridges of neutral gas that connect its members. One of the bridges forms a large tidal tail extending eastwards from NGC 3628 that hosts several H i plumes and carries the material from this galaxy to the intergalactic space. Aims. The magnetic fields of the member galaxies NGC 3628 and NGC 3627 show morphological peculiarities, suggesting that inter- actions within the group may be caused by stripping of the magnetic field. This process could supply the intergalactic space with magnetised material, a scenario considered as a possible source of intergalactic magnetic fields (as seen eg. in the “Taffy” pairs of galaxies). Additionally, the plumes are likely to be the tidal dwarf galaxy candidates. Methods. We performed radio continuum mapping observations at 2.64 GHz using the 100-m Effelsberg radio telescope. We obtained total power and polarised intensity maps of the Triplet. -
Observers' Forum
Observers’ Forum find M66 much the easier of the two Messier From the deep sky: the Leo Triplet galaxies in which to see detail, the bright north/south oval halo containing a condensed core which brightens gradually to the centre. Some of the detail that can be suspected visu- ally is shown in glorious detail in the image of M66 by Adrian Catterall, who observes from Royston in Hertfordshire. In addition to these Messier galaxies, Leo contains numerous other delights, in par- ticular a galaxy that Messier and his co- workers missed, the Sb/Sc spiral NGC 2903. This galaxy, which lies 1.5° south of magnitude 4.3 star λ Leo at the top of the ‘Sickle’ asterism, is a visual beauty. Dis- covered by William Herschel in November 1784 – presumably near the end of an all night observing session – it is visible in al- most any size of telescope and shows tre- mendous detail in a large aperture. It also images particularly well. The Director would be delighted to receive images and observations of NGC 2903, or of any of the other galaxies in Leo. Stewart L. Moore, Director, Deep Sky The Leo Triplet, M65, M66 & NGC 3628. TVNP101 APO refractor + Starlight Xpress Section HX916 CCD camera with ST4 autoguider. IDAS LPR filter & True Tech RGB colour filters. Image by Peter Carson. Lying due south around 21:00 UT in April, 3628 was discovered by the constellation of Leo is a recognisable William Herschel in 1783. grouping of stars even to people with only a These three galaxies all fit passing interest in astronomy. -
AYOSH Demo Chapter
DEMO CHAPTER Winter - January We start the year of Star Hopping at its beginning, in chilly January. By this point, I was 14 episodes into the Star Hopping series on YouTube, which was started in September. So that’s why we’re starting with Episode 14. We’ll roll over to Episode 1, nine months from now; in September. The months of Winter give rise to the brightest stars in the sky, anchored in the constellations of Orion, Canis Major, Canis Minor, and Gemini. In the northern climes, the weather may be frigid, but on those cold, clear nights, the stars shine more steadily, as the cold dry air makes for spectacular “seeing”. Chapter 4 - Leo We’ll be looking into the constellation of Leo for our Star Hopping targets in this chapter. I’ll be keeping you up a little later to around 11:30 PM, to see Leo the Lion appearing up over the eastern horizon. Even though we’re in January, we are A YEAR OF STAR HOPPING DAVID HEARN PAGE !1 OF !7 DEMO CHAPTER starting to get hints of the constellations of Spring starting to appear late in the evenings. This begins the time to see galaxies! The constellation of Leo portrays the great Lion, with the head of the lion appearing as a very recognizable backwards question mark, and the tail shaped like a large triangle. Leo rises with the head of the lion facing straight up, and within it’s borders lie many deep sky objects, most of which are as I mentioned, galaxies. -
Prime Focus (02-19).Pub
Highlights of the February Sky - - - 1st - - - AM: Antares, Jupiter, Venus, a waning crescent Moon, and Saturn form a 35° arc stretching from southeast to the south-southeast. - - - 4th - - - New Moon 4:04 pm EST KAS - - - 10th - - - PM: Aer sunset, look halfway up in the south- General Meeting: Friday, February 1 @ 7:00 pm southwest to see a waxing crescent Moon hanging Kalamazoo Area Math & Science Center - See Page 12 for Details some 6° lower le of Mars. - - - 12 - - - Observing: Saturday, February 2 @ 7:00 pm First Quarter Moon 5:26 pm EST February Freeze Out - Kalamazoo Nature Center DUSK: Mercury reemerges from superior conjuncon - look toward the west- Board Meeting: Sunday, February 10 @ 5:00 pm southwest aer sunset. Sunnyside Church - 2800 Gull Road - All Members Welcome - - - 13th - - - PM: The Moon is in the Hyades, 2° from Aldebaran. - - - 17th 19th - - - Inside the Newsletter. AM: Venus and Saturn are 1° apart. Look toward the southeast before sunrise. January Meeng Minutes.................. p. 2 Board Meeng Minutes..................... p. 2 - - - 17 - - - PM: A waxing gibbous Recent Addion to KAS Library.......... p. 3 Moon is in Cancer, next to Observaons...................................... p. 3 M44, the Beehive Cluster. Community Outreach in 2019............p. 4 - - - 26 - - - KAS Member Lunar Eclipse Images.... p. 5 Last Quarter Moon 6:28 am EST Tele Vue 32mm Plössl........................ p. 7 NASA Night Sky Notes........................ p. 8 - - - 27th - - - DAWN: A waning crescent Star Pares in 2019............................ p. 9 Moon is 2° to the upper February Night Sky............................. p. 10 right of Jupiter. KAS Board & Announcements............ p. 11 - - - 27th - - - DAWN: The Moon is about General Meeng Preview.................