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Umwandlungen im Insolvenzplanverfahren

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, Vol. 484



Untersuchungsgegenstand der Arbeit ist die Durchführung einer Umwandlung im Insolvenzplanverfahren. Eine Analyse kommt zu dem Ergebnis, dass die Einbindung einer Umwandlung ins Insolvenzplanverfahren seit ESUG gegen den Willen der Anteilsinhaber zulässig ist und es sich beim Schuldner regelmäßig um einen umwandlungsfähigen Rechtsträger handelt. Anschließend wird herausgearbeitet, wie eine Umwandlung im Insolvenzplanverfahren genau ablaufen kann. Dabei fällt inbesondere auf, dass die Einbindung ins Insolvenzplanverfahren zu zahlreichen Verfahrensvereinfachungen führt. Eine Analyse der Stellung der Anteilsinhaber bei einer Durchführung der Umwandlung im Insolvenzplanverfahren zeigt das Auftreten zahlreicher insolvenzplanrechtlicher Besonderheiten, die es zu beachten gilt. Die nähere Auseinandersetzung mit den Auswirkungen einer Einbindung auf die umwandlungsrechtlichen Gläubigerschutzvorschriften kommt zu dem Ergebnis, dass einige Vorschriften zulasten der Insolvenzgläubiger teleologisch zu reduzieren sind, andere hingegen weiterhin Anwendung finden müssen. »Conversions in the Insolvency Plan Procedure« This work discusses conversions in the insolvency plan procedure. A detailed analysis concludes that a conversion in the insolvency plan can be juristically included into the insolvency plan procedure against shareholder objectives since ESUG. Both how this change will be conducted and how it impacts the stance of shareholders is discussed. The examination of the wider implications on the creditor protection rules is a key aspect of the work.

About The Author

Cathrin Greif-Werner studied Law at the Johannes Gutenberg University Mainz, the Rheinische Friedrich-Wilhelms-University Bonn and the University of Cologne (PhD). After her first juridical state examination in 2015 she worked as a research associate at a german lawfirm. In June 2017 she started her legal clerkship in the higher regional court district Cologne. Cathrin Greif-Werner studierte Rechtswissenschaften an der Johannes Gutenberg Universität Mainz, der Rheinische Friedrich-Wilhelms-Universität Bonn und der Universität zu Köln (Dr.). Nach dem ersten juristischen Staatsexamen im Jahr 2015 war sie als wissenschaftliche Mitarbeiterin in einer deutschen Großkanzlei tätig. Seit Juni 2017 absolviert sie ihr Referendariat im OLG-Bezirk Köln.


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eso1814 — Science Release

9 May 2018

An international team of astronomers has used ESO telescopes to investigate a relic of the primordial Solar System. The team found that the unusual Kuiper Belt Object 2004 EW95 is a carbon-rich asteroid, the first of its kind to be confirmed in the cold outer reaches of the Solar System. This curious object likely formed in the asteroid belt between Mars and Jupiter and has been flung billions of kilometres from its origin to its current home in the Kuiper Belt.

The early days of our Solar System were a tempestuous time. Theoretical models of this period predict that after the gas giants formed they rampaged through the Solar System, ejecting James Low Top Sneakers Sale Cheap Price View For Sale Outlet Good Selling Many Kinds Of Cheap Online Explore 7hMY9a
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. In particular, these models suggest that the Kuiper Belt — a cold region beyond the orbit of Neptune — should contain a small fraction of rocky bodies from the inner Solar System, such as carbon-rich asteroids, referred to as DURAMO Pool sliders black/white Wide Range Of Cheap Online Cheap Buy Best Store To Get Cheap Online Free Shipping Sale Online unIMNOH
[2] .

Now, a recent paper has presented evidence for the first reliably-observed carbonaceous asteroid in the Kuiper Belt, providing strong support for these theoretical models of our Solar System’s troubled youth. After painstaking measurements from multiple instruments at ESO’s Very Large Telescope (VLT), a small team of astronomers led by Tom Seccull of Queen’s University Belfast in the UK was able to measure the composition of the anomalous Kuiper Belt Object 2004 EW 95 , and thus determine that it is a carbonaceous asteroid. This suggests that it originally formed in the inner Solar System and must have since migrated outwards [3] .

The peculiar nature of 2004 EW 95 first came to light during routine observations with the NASA/ESA Hubble Space Telescope by Wesley Fraser, an astronomer from Queen’s University Belfast who was also amember of the team behind this discovery. The asteroid’s Free Shipping Pay With Paypal Converse Chuck Taylor® All Star® II Shield Canvas Hi Cheap Pay With Visa Discount In China Buy Cheap Low Price Pictures Cheap Online 6KLFTXQu9
— the specific pattern of wavelengths of light reflected from an object — was different to that of similar small Kuiper Belt Objects (KBOs), which typically have uninteresting, featureless spectra that reveal little information about their composition.

The reflectance spectrum of 2004 EW 95 was clearly distinct from the other observed outer Solar System objects, ” explains lead author Seccull. “ It looked enough of a weirdo for us to take a closer look.

The team observed 2004 EW 95 with the X-Shooter and FORS2 instruments on the VLT. The sensitivity of these spectrographs allowed the team to obtain more detailed measurements of the pattern of light reflected from the asteroid and thus infer its composition.

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