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Sentimental Appropriations: Contemporary Sympathy In
SENTIMENTAL APPROPRIATIONS: CONTEMPORARY SYMPATHY IN THE NOVELS OF GRACE LUMPKIN, JOSEPHINE JOHNSON, JOHN STEINBECK, MARGARET WALKER, OCTAVIA BUTLER, AND TONI MORRISON Jennifer A. Williamson A dissertation submitted to the faculty of the University of North Carolina in partial fulfillment of the requirements for the degree of Doctor of Philosophy in the Department of English and Comparative Literature Chapel Hill 2011 Approved by: Linda Wagner-Martin William L. Andrews Philip Gura Fred Hobson Wahneema Lubiano © 2011 Jennifer A. Williamson ALL RIGHTS RESERVED ii ABSTRACT JENNIFER A. WILLIAMSON: Sentimental Appropriations: Contemporary Sympathy in the Novels of Grace Lumpkin, Josephine Johnson, John Steinbeck, Margaret Walker, Octavia Butler, and Toni Morrison (Under the direction of Linda Wagner-Martin) This project investigates the appearance of the nineteenth-century American sentimental mode in more recent literature, revealing that the cultural work of sentimentalism continues in the twentieth-century and beyond. By examining working-class literature that adopts the rhetoric of “feeling right” in order to promote a proletarian ideology as well as neo-slave narratives that wrestle with the legacy of slavery, this study explores the ways contemporary authors engage with familiar sentimental tropes and ideals. Despite modernism’s influential assertion that sentimentalism portrays emotion that lacks reality or depth, narrative claims to feeling— particularly those based in common and recognizable forms of suffering—remain popular. It seems clear that such authors as Grace Lumpkin, Josephine Johnson, John Steinbeck, Margaret Walker, Octavia Butler, and Toni Morrison apply the rhetorical methods of sentimentalism to the cultural struggles of their age. Contemporary authors self-consciously struggle with sentimentalism’s gender, class, and race ideals; however, sentimentalism’s dual ability to promote these ideals and extend identification across them makes it an attractive and effective mode for political and social influence. -
Difference, Identification, Evolution
DIFFERENCE, IDENTIFICATION, EVOLUTION: POSTHUMANISM AS PARADIGMATIC SHIFT IN CONTEMPORARY SPECULATIVE FICTION BY BETHANY DOANE A THESIS IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF MASTER OF ARTS IN HUMANITIES DEPARTMENT OF ENGLISH TOWSON UNIVERSITY TOWSON, MARYLAND 21252 MAY, 2013 ii ACKNOWLEDGEMENTS This thesis would not have been possible without the support and encouragement of Dr. Jennifer Ballengee, who served not only as a committee chair, but also as a mentor, editor, and friend during the research and composition of this project. I would also like to thank Dr. George Hahn, Dr. Erin Fehskens, and Dr. Peter Baker, who also provided guidance and advice throughout the writing process. Lastly, I would like to give special thanks to my husband, Jeff, (who was not yet my husband when this project started) for putting up with me and my many neurotic research and writing habits. Thank you all so much. ii ABSTRACT Difference, Identification, Evolution: Posthumanism as Paradigmatic Shift in Contemporary Speculative Fiction Bethany Doane This study is an initial attempt to investigate the ways that posthumanism manifests within three works of contemporary speculative fiction: Margaret Atwood’s Oryx and Crake (2010), Kazuo Ishiguro’s Never Let Me Go (2005) and Richard Powers’s Galatea 2.2 (1995). Posthumanism seeks to overturn the assumptions of liberal humanism, which places “the human” as the central, most important, and possibly only ethical subject in order to recognize inhuman beings—whether they be animal, clone, or artificial intelligence—as legitimate ethical subjects. At the same time, it recognizes that human beings and technology are intimately bound together. -
A New Universe to Discover: a Guide to Careers in Astronomy
A New Universe to Discover A Guide to Careers in Astronomy Published by The American Astronomical Society What are Astronomy and Astrophysics? Ever since Galileo first turned his new-fangled one-inch “spyglass” on the moon in 1609, the popular image of the astronomer has been someone who peers through a telescope at the night sky. But astronomers virtually never put eye to lens these days. The main source of astronomical data is still photons (particles of light) from space, but the tools used to gather and analyze them are now so sophisticated that it’s no longer necessary (or even possible, in most cases) for a human eye to look through them. But for all the high-tech gadgetry, the 21st-Century astronomer is still trying to answer the same fundamental questions that puzzled Galileo: How does the universe work, and where did it come from? Webster’s dictionary defines “astronomy” as “the science that deals with the material universe beyond the earth’s atmosphere.” This definition is broad enough to include great theoretical physicists like Isaac Newton, Albert Einstein, and Stephen Hawking as well as astronomers like Copernicus, Johanes Kepler, Fred Hoyle, Edwin Hubble, Carl Sagan, Vera Rubin, and Margaret Burbidge. In fact, the words “astronomy” and “astrophysics” are pretty much interchangeable these days. Whatever you call them, astronomers seek the answers to many fascinating and fundamental questions. Among them: *Is there life beyond earth? *How did the sun and the planets form? *How old are the stars? *What exactly are dark matter and dark energy? *How did the Universe begin, and how will it end? Astronomy is a physical (non-biological) science, like physics and chemistry. -
Appendix: Spectroscopy of Variable Stars
Appendix: Spectroscopy of Variable Stars As amateur astronomers gain ever-increasing access to professional tools, the science of spectroscopy of variable stars is now within reach of the experienced variable star observer. In this section we shall examine the basic tools used to perform spectroscopy and how to use the data collected in ways that augment our understanding of variable stars. Naturally, this section cannot cover every aspect of this vast subject, and we will concentrate just on the basics of this field so that the observer can come to grips with it. It will be noticed by experienced observers that variable stars often alter their spectral characteristics as they vary in light output. Cepheid variable stars can change from G types to F types during their periods of oscillation, and young variables can change from A to B types or vice versa. Spec troscopy enables observers to monitor these changes if their instrumentation is sensitive enough. However, this is not an easy field of study. It requires patience and dedication and access to resources that most amateurs do not possess. Nevertheless, it is an emerging field, and should the reader wish to get involved with this type of observation know that there are some excellent guides to variable star spectroscopy via the BAA and the AAVSO. Some of the workshops run by Robin Leadbeater of the BAA Variable Star section and others such as Christian Buil are a very good introduction to the field. © Springer Nature Switzerland AG 2018 M. Griffiths, Observer’s Guide to Variable Stars, The Patrick Moore 291 Practical Astronomy Series, https://doi.org/10.1007/978-3-030-00904-5 292 Appendix: Spectroscopy of Variable Stars Spectra, Spectroscopes and Image Acquisition What are spectra, and how are they observed? The spectra we see from stars is the result of the complete output in visible light of the star (in simple terms). -
An International Journal of English Studies 25/1 2016 EDITOR Prof
ANGLICA An International Journal of English Studies 25/1 2016 EDITOR prof. dr hab. Grażyna Bystydzieńska [[email protected]] ASSOCIATE EDITORS dr hab. Marzena Sokołowska-Paryż [[email protected]] dr Anna Wojtyś [[email protected]] ASSISTANT EDITORS dr Katarzyna Kociołek [[email protected]] dr Magdalena Kizeweter [[email protected]] ADVISORY BOARD GUEST REVIEWERS Michael Bilynsky, University of Lviv Dorota Babilas, University of Warsaw Andrzej Bogusławski, University of Warsaw Teresa Bela, Jagiellonian University, Cracow Mirosława Buchholtz, Nicolaus Copernicus University, Toruń Maria Błaszkiewicz, University of Warsaw Xavier Dekeyser University of Antwerp / KU Leuven Anna Branach-Kallas, Nicolaus Copernicus University, Toruń Bernhard Diensberg, University of Bonn Teresa Bruś, University of Wrocław, Poland Edwin Duncan, Towson University, Towson, MD Francesca de Lucia, independent scholar Jacek Fabiszak, Adam Mickiewicz University, Poznań Ilona Dobosiewicz, Opole University Jacek Fisiak, Adam Mickiewicz University, Poznań Andrew Gross, University of Göttingen Elzbieta Foeller-Pituch, Northwestern University, Evanston-Chicago Paweł Jędrzejko, University of Silesia, Sosnowiec Piotr Gąsiorowski, Adam Mickiewicz University, Poznań Aniela Korzeniowska, University of Warsaw Keith Hanley, Lancaster University Andrzej Kowalczyk, Maria Curie-Skłodowska University, Lublin Christopher Knight, University of Montana, Missoula, MT Barbara Kowalik, University of Warsaw Marcin Krygier, Adam Mickiewicz University, Poznań Ewa Łuczak, University of Warsaw Krystyna Kujawińska-Courtney, University of Łódź David Malcolm, University of Gdańsk Zbigniew Mazur, Maria Curie-Skłodowska University, Lublin Dominika Oramus University of Warsaw Znak ogólnodostępnyRafał / Molencki,wersje University językowe of Silesia, Sosnowiec Marek Paryż, University of Warsaw John G. Newman, University of Texas at Brownsville Anna Pochmara, University of Warsaw Michal Jan Rozbicki, St. -
GEORGE HERBIG and Early Stellar Evolution
GEORGE HERBIG and Early Stellar Evolution Bo Reipurth Institute for Astronomy Special Publications No. 1 George Herbig in 1960 —————————————————————– GEORGE HERBIG and Early Stellar Evolution —————————————————————– Bo Reipurth Institute for Astronomy University of Hawaii at Manoa 640 North Aohoku Place Hilo, HI 96720 USA . Dedicated to Hannelore Herbig c 2016 by Bo Reipurth Version 1.0 – April 19, 2016 Cover Image: The HH 24 complex in the Lynds 1630 cloud in Orion was discov- ered by Herbig and Kuhi in 1963. This near-infrared HST image shows several collimated Herbig-Haro jets emanating from an embedded multiple system of T Tauri stars. Courtesy Space Telescope Science Institute. This book can be referenced as follows: Reipurth, B. 2016, http://ifa.hawaii.edu/SP1 i FOREWORD I first learned about George Herbig’s work when I was a teenager. I grew up in Denmark in the 1950s, a time when Europe was healing the wounds after the ravages of the Second World War. Already at the age of 7 I had fallen in love with astronomy, but information was very hard to come by in those days, so I scraped together what I could, mainly relying on the local library. At some point I was introduced to the magazine Sky and Telescope, and soon invested my pocket money in a subscription. Every month I would sit at our dining room table with a dictionary and work my way through the latest issue. In one issue I read about Herbig-Haro objects, and I was completely mesmerized that these objects could be signposts of the formation of stars, and I dreamt about some day being able to contribute to this field of study. -
Abstracts of Talks 1
Abstracts of Talks 1 INVITED AND CONTRIBUTED TALKS (in order of presentation) Milky Way and Magellanic Cloud Surveys for Planetary Nebulae Quentin A. Parker, Macquarie University I will review current major progress in PN surveys in our own Galaxy and the Magellanic clouds whilst giving relevant historical context and background. The recent on-line availability of large-scale wide-field surveys of the Galaxy in several optical and near/mid-infrared passbands has provided unprecedented opportunities to refine selection techniques and eliminate contaminants. This has been coupled with surveys offering improved sensitivity and resolution, permitting more extreme ends of the PN luminosity function to be explored while probing hitherto underrepresented evolutionary states. Known PN in our Galaxy and LMC have been significantly increased over the last few years due primarily to the advent of narrow-band imaging in important nebula lines such as H-alpha, [OIII] and [SIII]. These PNe are generally of lower surface brightness, larger angular extent, in more obscured regions and in later stages of evolution than those in most previous surveys. A more representative PN population for in-depth study is now available, particularly in the LMC where the known distance adds considerable utility for derived PN parameters. Future prospects for Galactic and LMC PN research are briefly highlighted. Local Group Surveys for Planetary Nebulae Laura Magrini, INAF, Osservatorio Astrofisico di Arcetri The Local Group (LG) represents the best environment to study in detail the PN population in a large number of morphological types of galaxies. The closeness of the LG galaxies allows us to investigate the faintest side of the PN luminosity function and to detect PNe also in the less luminous galaxies, the dwarf galaxies, where a small number of them is expected. -
Astronomical Coordinate Systems
Appendix 1 Astronomical Coordinate Systems A basic requirement for studying the heavens is being able to determine where in the sky things are located. To specify sky positions, astronomers have developed several coordinate systems. Each sys- tem uses a coordinate grid projected on the celestial sphere, which is similar to the geographic coor- dinate system used on the surface of the Earth. The coordinate systems differ only in their choice of the fundamental plane, which divides the sky into two equal hemispheres along a great circle (the fundamental plane of the geographic system is the Earth’s equator). Each coordinate system is named for its choice of fundamental plane. The Equatorial Coordinate System The equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the most closely related to the geographic coordinate system because they use the same funda- mental plane and poles. The projection of the Earth’s equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles onto the celestial sphere defines the north and south celestial poles. However, there is an important difference between the equatorial and geographic coordinate sys- tems: the geographic system is fixed to the Earth and rotates as the Earth does. The Equatorial system is fixed to the stars, so it appears to rotate across the sky with the stars, but it’s really the Earth rotating under the fixed sky. The latitudinal (latitude-like) angle of the equatorial system is called declination (Dec. for short). It measures the angle of an object above or below the celestial equator. -
THE OBSERVER MAY 10, 2021 NOTE from the DIRECTOR Dear
THE OBSERVER MAY 10, 2021 NOTE FROM THE DIRECTOR Dear all, Thank you to those who attended the General Membership Meeting on Friday afternoon – and for your positive feedback! Videos and photos will be added to the list of things to carry forward from Zoom life into in-person presenting, working, and learning. For those who missed it (or who want to relive it!) we recorded the meeting and it can be watched HERE (insert link). Another reminder that registration for summer session (June 1- July 12) closes today at 5PM. All summer study groups will be held on Zoom and the fees are $125 for one study group and $200 for two or three study groups. The Summer Grid is here and Registration form here. Fall registration is open until May 14 (this Friday) for current members. The Fall Grid is here: and the Registration form here: We will inform you about which study groups will have an in-person option as soon as we have secured the classrooms with the Registrar. Thank you for your patience and flexibility as we take these next steps. While this is the last regular issue of The Observer for the semester, please keep a look out for special editions with updates. In addition to summer study groups, some programming is ongoing including the newly minted Science Series (read on for details) and workshops for coordinators. The Advisory Board and I are continuing the development of a new workshop for coordinators to provide strategies towards implementation of the program’s commitment to diversity, equity, and inclusion with the mission of fostering an environment of trust and respect while bringing to light, and more closely examining, how words and actions affect a climate of inclusion for all. -
Sentimental Appropriations
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Carolina Digital Repository SENTIMENTAL APPROPRIATIONS: CONTEMPORARY SYMPATHY IN THE NOVELS OF GRACE LUMPKIN, JOSEPHINE JOHNSON, JOHN STEINBECK, MARGARET WALKER, OCTAVIA BUTLER, AND TONI MORRISON Jennifer A. Williamson A dissertation submitted to the faculty of the University of North Carolina in partial fulfillment of the requirements for the degree of Doctor of Philosophy in the Department of English and Comparative Literature Chapel Hill 2011 Approved by: Linda Wagner-Martin William L. Andrews Philip Gura Fred Hobson Wahneema Lubiano © 2011 Jennifer A. Williamson ALL RIGHTS RESERVED ii ABSTRACT JENNIFER A. WILLIAMSON: Sentimental Appropriations: Contemporary Sympathy in the Novels of Grace Lumpkin, Josephine Johnson, John Steinbeck, Margaret Walker, Octavia Butler, and Toni Morrison (Under the direction of Linda Wagner-Martin) This project investigates the appearance of the nineteenth-century American sentimental mode in more recent literature, revealing that the cultural work of sentimentalism continues in the twentieth-century and beyond. By examining working-class literature that adopts the rhetoric of “feeling right” in order to promote a proletarian ideology as well as neo-slave narratives that wrestle with the legacy of slavery, this study explores the ways contemporary authors engage with familiar sentimental tropes and ideals. Despite modernism’s influential assertion that sentimentalism portrays emotion that lacks reality or depth, narrative claims to feeling— particularly those based in common and recognizable forms of suffering—remain popular. It seems clear that such authors as Grace Lumpkin, Josephine Johnson, John Steinbeck, Margaret Walker, Octavia Butler, and Toni Morrison apply the rhetorical methods of sentimentalism to the cultural struggles of their age. -
A New Universe to Discover: a Guide to Careers in Astronomy
A New Universe to Discover A Guide to Careers in Astronomy Published by The American Astronomical Society What are Astronomy and Astrophysics? Ever since Galileo first turned his new-fangled one-inch “spyglass” on the moon in 1609, the popular image of the astronomer has been someone who peers through a telescope at the night sky. But astronomers virtually never put eye to lens these days. The main source of astronomical data is still photons (particles of light) from space, but the tools used to gather and analyze them are now so sophisticated that it’s no longer necessary (or even possible, in most cases) for a human eye to look through them. But for all the high-tech gadgetry, the 21st-Century astronomer is still trying to answer the same fundamental questions that puzzled Galileo: How does the universe work, and where did it come from? Webster’s dictionary defines “astronomy” as “the science that deals with the material universe beyond the earth’s atmosphere.” This definition is broad enough to include great theoretical physicists like Isaac Newton, Albert Einstein, and Stephen Hawking as well as astronomers like Copernicus, Johanes Kepler, Fred Hoyle, Edwin Hubble, Carl Sagan, Vera Rubin, and Margaret Burbidge. In fact, the words “astronomy” and “astrophysics” are pretty much interchangeable these days. Whatever you call them, astronomers seek the answers to many fascinating and fundamental questions. Among them: *Is there life beyond earth? *How did the sun and the planets form? *How old are the stars? *What exactly are dark matter and dark energy? *How did the Universe begin, and how will it end? Astronomy is a physical (non-biological) science, like physics and chemistry. -
One of the Most Interactive and Inspiring Exhibitions
RIDE IN A LIVE-ACTION SNOWBOARD RACE, CONTROL A MARS ROVER, DESIGN AND PLAY YOUR OWN VIDEO GAME, CAPTURE YOUR IMAGE IN A 360 FREEZE-MOTION VIDEO. EXPERIENCE REAL MATH AT WORK IN SPORTS, NATURE, ROBOTICS, MUSIC, DANCING, MOVIE-MAKING AND MORE. 40 IMMERSIVE INTERACTIVE EXHIBITS. MATH HAS NEVER BEEN SO SWEET! AT A GLANCE • EXHIBIT SIZE: 5,000 SQUARE FEET (500 SQUARE METERS) • TARGET AUDIENCE: FAMILIES, STUDENTS GRADES K – 12 (FOCUS ON GRADES 3 – 8, AGES 7 – 14) • LENGTH OF VENUE: APPROXIMATELY THREE MONTHS SPRING, SUMMER, FALL • PREMIERED AT THE SMITHSONIAN No exhibition ever has better The institutional partners will be available to support host ONE OF THE MOST museums, with varying types of events, competitions and answered the age-old question: activities throughout the live schedule, helping host museums turn entire cities into ‘math towns’ with rich calendars of INTERACTIVE activities throughout the run of the exhibition. From special live competitions to STEM career events, the supplemental “Will I ever use all AND INSPIRING resources, media, materials, events and programming will EXHIBITIONS EXPLORING support museums in bringing math meaningfully and this math they’re effectively into their larger experience. This innovative exhibit responds to the national movement teaching us?” THE WORLD toward greater focus on STEM development and STEM career awareness, and inspiring kids to make math a priority, OF MATHEMATICS reaching them in that window of vulnerability when math gets more challenging and kids begin to lose interest. MathAlive! is designed to inspire, to spark the imagination, to reveal not only math at work, but the endless possibilities MathAlive! is produced by Evergreen Exhibitions and of math.