The Mice at play in the CALIFA survey. A case study of a gas-rich major merger between first passage and coalescence

We present optical integral field spectroscopy (IFS) observations of the Mice, a major merger between two massive (≳10^11 M_⊙) gas-rich spirals NGC 4676A and B, observed between first passage and final coalescence. The spectra provide stellar and gas kinematics, ionised gas properties, and stellar population diagnostics, over the full optical extent of both galaxies with ~1.6 kpc spatial resolution. The Mice galaxies provide a perfect case study that highlights the importance of IFS data for improving our understanding of local galaxies. The impact of first passage on the kinematics of the stars and gas has been significant, with strong bars most likely induced in both galaxies. The barred spiral NGC 4676B exhibits a strong twist in both its stellar and ionised gas disk. The edge-on disk galaxy NGC 4676A appears to be bulge free, with a strong bar causing its “boxy” light profile. On the other hand, the impact of the merger on the stellar populations has been minimal thus far. By combining the IFS data with archival multiwavelength observations we show that star formation induced by the recent close passage has not contributed significantly to the total star formation rate or stellar mass of the galaxies. Both galaxies show bicones of high ionisation gas extending along their minor axes. In NGC 4676A the high gas velocity dispersion and Seyfert-like line ratios at large scaleheight indicate a powerful outflow. Fast shocks (vs ~ 350 km s^-1) extend to ~6.6 kpc above the disk plane. The measured ram pressure (P/k = 4.8 × 10^6 K cm^-3) and mass outflow rate (~8−20 M_⊙ yr^-1) are similar to superwinds from local ultra-luminous infrared galaxies, although NGC 4676A only has a moderate infrared luminosity of 3 × 10^10 L_⊙. Energy beyond what is provided by the mechanical energy of the starburst appears to be required to drive the outflow. Finally, we compare the observations to mock kinematic and stellar population maps extracted from a hydrodynamical merger simulation. The models show little enhancement in star formation during and following first passage, in agreement with the observations. We highlight areas where IFS data could help further constrain the models.

The merger history of massive spheroids since z ∼ 1 is size independent

Using a compilation of 379 massive (stellar mass M ≳ 10^11 M_⊙) spheroid-like galaxies from the near-infrared Palomar/DEEP-2 survey, we investigated, up to z ∼ 1, whether the presence of companions depends on the size of the host galaxy. We explored the presence of companions for mass ratios with respect to the central massive galaxy down to 1 : 10 and 1 : 100, and within projected distances of 30, 50 and 100 kpc of these objects. We found evidence that these companions are equally distributed around both compact and extended massive spheroid-like galaxies. This suggests that, at least since z ∼ 1, the merger activity in these objects is nearly homogeneous across the whole population and that the merger history is not affected by the size of the host galaxy. Our results could indicate that compact and extended massive spheroid-like galaxies are increasing in size at the same rate.

MY Camelopardalis, a very massive merger progenitor

Context. The early-type binary MY Cam belongs to the young open cluster Alicante 1, embedded in Cam OB3. Aims. MY Cam consists of two early-O type main-sequence stars and shows a photometric modulation suggesting an orbital period slightly above one day. We intend to confirm this orbital period and derive orbital and stellar parameters. Methods. Timing analysis of a very exhaustive (4607 points) light curve indicates a period of 1.1754514 ± 0.0000015 d. High-resolution spectra and the cross-correlation technique implemented in the todcor program were used to derive radial velocities and obtain the corresponding radial velocity curves for MY Cam. Modelling with the stellar atmosphere code fastwind was used to obtain stellar parameters and create templates for cross-correlation. Stellar and orbital parameters were derived using the Wilson-Devinney code, such that a complete solution to the binary system could be described. Results. The determined masses of the primary and secondary stars in MY Cam are 37.7 ± 1.6 and 31.6 ± 1.4M⊙, respectively. The corresponding temperatures, derived from the model atmosphere fit, are 42 000 and 39 000 K, with the more massive component being hotter. Both stars are overfilling their Roche lobes, sharing a common envelope. Conclusions. MY Cam contains the most massive dwarf O-type stars found so far in an eclipsing binary. Both components are still on the main sequence, and probably not far from the zero-age main sequence. The system is a likely merger progenitor, owing to its very short period.

Le contrôle européen des concentrations et les leçons à tirer de la crise financière et économique = European merger control and the lessons of the financial and economic crisis. Research Papers in Law, 06/2013

No abstract.

The Standard of Proof in EC Merger Control-Conclusions from the Sony BMG Saga. IES WORKING PAPER 4/2008

One of the most important developments in EC competition policy during 2006 was the Court of First Instance’s (CFI) Impala v. Commission judgment annulling the European Commission’s approval of the merger between the music units of Sony and Bertelsmann. It harshly criticized the Commission’s Decision because it found that the evidence relied on was not capable of substantiating the conclusion. This was the first time that a merger decision was annulled for not meeting the requisite legal standard for authorizing the merger. Consequently, the CFI raised fundamental questions about the standard of proof incumbent on the Commission in its merger review procedures. On July 10, 2008, the European Court of Justice overturned Impala, yet it did not resolve the fundamental question underlying the judicial review of the Sony BMG Decision; does the Commission have the necessary resources and expertise to meet the Community Court’s standard of proof? This paper addresses the wider implications of the Sony BMG saga for the Commission’s future handling of complex merger investigations. It argues that the Commission may have set itself an impossible precedent in the second approval of the merger. While the Commission has made a substantial attempt to meet the high standard of proof imposed by the Community Courts, it is doubtful that it will be able to jump the fence again in a similar fashion under normal procedural circumstances.

Controlled ‘Europeanisation’? The KMW–Nexter merger and the Germany’s new strategy for the arms industry. OSW COMMENTARY NUMBER 180/26.08.2015

On 29 July a deal was signed in Paris concerning a merger between Krauss-Maffei Wegmann (KMW), Germany’s largest manufacturer of tanks, infantry fighting vehicles and artillery systems, and its French counterpart Nexter. The new holding formed as a result of the merger will be Europe’s largest producer of arms systems for land forces, comparable to the Airbus Group in the aerospace industry. While work on finalising the merger was underway, the German government was developing a new strategy for Germany’s arms industry, which was published on 9 June 2015. The strategy’s provisions show that German politicians, despite holding negative opinions on previous mergers between German arms companies and foreign businesses, have concluded that consolidation at the European level is nonetheless the only way to go. However, the strategy also states that the German government should exercise more influence than previously on the terms and conditions of any such consolidation. To this end, it identified key national technologies which will be supported and protected through various instruments, including also the conclusion of intergovernmental agreements on strategic defence co-operation. Such agreements may regulate questions such as the ownership structures of the new companies, the locations for developing technologies and for manufacturing products, subcontractors and exports of jointly developed arms and military equipment. In relation to the KMW–Nexter merger, such a deal between France and Germany is expected to be signed this autumn.

Rail merger legislation. Hearings, Eighty-seventh Congress, second session, pursuant to S. Res. 258 on S. 3097.

Mode of access: Internet.

The fall of a railroad empire; Brandeis and the New Haven merger battle,

"Bibliographical note": p. 205-209.