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Author: Edward J. Wood
Publisher: BoD – Books on Demand
ISBN: 3752514450
Category : Fiction
Languages : en
Pages : 490
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Book Description
Reprint of the original, first published in 1868.
Author: Edward J. Wood
Publisher: BoD – Books on Demand
ISBN: 3752514450
Category : Fiction
Languages : en
Pages : 490
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Book Description
Reprint of the original, first published in 1868.
Author: Edward J. Wood
Publisher:
ISBN:
Category : Abnormalities, Human
Languages : en
Pages : 498
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Book Description
Author: Yehuda Koren
Publisher:
ISBN: 9781849546539
Category : Dwarfs
Languages : en
Pages : 283
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Book Description
In this account of the Ovitz family, seven of whose ten members were dwarves, readers bear witness to the terrible irony of the Ovitzs' fate: being burdened with dwarfism helped them to endure the Holocaust. Through research and interviews with the youngest Ovitz daughter, Perla, the troupe's last surviving member, and other relatives, the authors weave the tale of a beloved and successful family of performers who were famous entertainers in Central Europe until the Nazis deported them to Auschwitz in May 1944.
Author: ROBERT JASTROW
Publisher:
ISBN:
Category :
Languages : en
Pages : 262
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Book Description
Author: Peter Stabel
Publisher:
ISBN:
Category : Business & Economics
Languages : en
Pages : 316
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Book Description
Author: Edward J. Wood
Publisher:
ISBN: 9780841496095
Category : Dwarfs
Languages : en
Pages : 472
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Book Description
Author: Wood Edward J.
Publisher:
ISBN: 9780243824700
Category :
Languages : en
Pages :
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Book Description
Author: Robert Jastrow
Publisher: W. W. Norton & Company
ISBN: 9780393850048
Category : Fiction
Languages : en
Pages : 488
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Book Description
Presents discussions regarding the origin of the universe, the life and death of stars and the origin of the earth and life.
Author: Yehuda Koren
Publisher: Hachette+ORM
ISBN: 0786738561
Category : History
Languages : en
Pages : 338
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Book Description
In this remarkable, never-before-told account of the Ovitz family, seven of whose ten members were dwarves, readers bear witness to the best and worst of humanity and to the terrible irony of the Ovitz's fate: being burdened with dwarfism helped them endure the Holocaust. Israeli authors Yehuda Koren and Eilat Negev weave the tale of a beloved and successful family of performers who were famous entertainers in Central Europe until the Nazis deported them to Auschwitz in May 1944. Descending into the hell of the concentration camp from the transport train, the Ovitz family—known widely as the Lilliput Troupe—was separated from other Jewish victims. Dr. Josef Mengele was notified of their arrival and they were assigned better quarters and provided more nutritious food than other inmates. The authors chronicle Mengele's experiments upon the Ovitz's, and the creepy fondness he developed for these small people, even the songs he composed and sang to this family of singers, dancers, and klezmorim. Finally liberated by Russian troops, the family returned to their deserted village in Transylvania, and eventually found their way to a new home in Israel. They resumed their careers, overcame their handicaps and became wealthy and successful performers.
Author: Clare Higgs
Publisher:
ISBN:
Category :
Languages : en
Pages :
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Book Description
This thesis attempts to untangle, as best as possible, the importance of internally-driven evolutionary mechanisms relative to externally-driven effects, in shaping the structure and properties of the smallest observable galaxies. All galaxies are influenced by internal processes, such as feedback from star formation and the infall of gas or lack thereof, as well as environmental processes, like tides and ram pressure stripping. The smallest galaxies - dwarfs - are highly susceptible to all such processes, and their resulting structure is the summation of all prior events. I use nearby dwarf galaxies of the Local Group as test cases, focusing on those which are separated from the massive galaxies (like the Milky Way) and can be considered as "isolated''. These dwarfs are observed as part of the Solitary Local (Solo) Dwarf Galaxy Survey. Solo dwarfs will have spent the majority of their time as isolated systems, hence their properties should generally reflect their "intrinsic nature", unperturbed and unaffected by interactions with other systems. This survey was designed to focus on the old stellar populations present in these galaxies, in order to characterize their faint and extended structures. These old stellar populations should carry the hallmarks of the dwarfs' histories. By comparing the observed properties of Solo dwarfs with dwarfs currently in close proximity to a large host galaxy (i.e., the M 31 and Milky Way satellites), it should be possible to determine what aspects of the properties of dwarfs are most affected by environmentally-driven processes. The Local Group is the ideal regime in which to study these faint features, as the dwarfs' close proximity to us presents an opportunity to fully characterize these galaxies. However, the number of dwarfs in the Local Group is limited, with several galaxies (e.g. IC 10 or Sag dSph) being the unique example of their "type" locally observable. This limited sample emphasizes the need for careful, homogeneous observations and analysis, such that comparisons between this small, yet highly diverse, snapshot of galaxies accurately reflects the true nature of these dwarfs. I have homogeneously analyzed the 12 closest Solo dwarfs observable from the northern hemisphere, resulting in a consistently derived dataset. I determine fundamental properties, like distances, and characterize the structure of the dwarfs. I explore the possibility that the dwarfs may be more consistent with a two component profile, rather than one, finding that they are largely well characterized by a single Sérsic profile. I then compare these isolated dwarfs with the well-studied satellites of the Milky Way and M 31, primarily using two other homogeneous surveys; the MegaCam Survey of Outer Halo Objects and the Pan-Andromeda Archaeological Survey respectively. Examining each property (e.g. ellipticity, central surface brightness, or Sérsic radius) individually, we find no statistically significant differences between each group. However, when considering parameters in combination (e.g. absolute magnitude as a function of Sérsic radius), we see increased scatter in the satellite population, indicative of the impact of a massive host galaxy on the dwarfs, likely via tidal effects. The comparison between satellites and isolated dwarfs hones in on the impact of a massive galaxy in close proximity. Of course, processes within and surrounding the dwarf itself can also alter the dwarf. I look at the star formation histories and gas content of the dwarfs to explore the connection between internal and external processes in these small galaxies. Finally, I search for substructure in the form of satellites of dwarf galaxies, globular clusters and extended tidal features, all which inform about the dwarf's isolation, environment and history. Collectively, I generate comprehensive and detailed inspections of Local Group dwarfs and aim to understand them as products of their environment.
