TY - JOUR A1 - Bubner, Ben A1 - Buchheit, Ramona A1 - Friedrich, Frank A1 - Kummer, Volker A1 - Scholler, Markus T1 - Species identification of European forest pathogens of the genus Milesina (Pucciniales) using urediniospore morphology and molecular barcoding including M. woodwardiana sp. nov. JF - MycoKeys N2 - Species of rust fungi of the genus Milesina (Pucciiastraceae, Pucciniales) are distributed mainly in northern temperate regions. They host-alternate between needles of fir (Abies spp.) and fronds of ferns (species of Polypodiales). Milesina species are distinguished based on host taxonomy and urediniospore morphology. In this study, 12 species of Milesina from Europe were revised. Specimens were examined by light and scanning electron microscopy for urediniospore morphology with a focus on visualising germ pores (number, size and position) and echinulation. In addition, barcode loci (ITS, nad6, 28S) were used for species delimitation and for molecular phylogenetic analyses. Barcodes of 72 Milesina specimens were provided, including 11 of the 12 species. Whereas urediniospore morphology features were sufficient to distinguish all 12 Milesina species except for 2 (M. blechni and M. kriegeriana), ITS sequences separated only 4 of 11 species. Sequencing with 28S and nad6 did not improve species resolution. Phylogenetic analysis, however, revealed four phylogenetic groups within Milesina that also correlate with specific urediniospore characters (germ pore number and position and echinulation). These groups are proposed as new sections within Milesina (sections Milesina, Vogesiacae M. Scholler & Bubner, sect. nov., Scolopendriorum M. Scholler & Bubner, sect. nov. and Carpaticae M. Scholler & Bubner, sect. nov.). In addition, Milesina woodwardiana Buchheit & M. Scholler, sp. nov. on Woodwardia radicans, a member of the type section Milesina, is newly described. An identification key for European Milesina species, based on urediniospore features, is provided. KW - Abies alba KW - Polypodiales KW - GBOL KW - germ pores KW - host alternation KW - Uredinopsis KW - Europe Y1 - 2019 U6 - https://doi.org/10.3897/mycokeys.48.30350 SN - 1314-4057 SN - 1314-4049 IS - 48 SP - 1 EP - 40 PB - Pensoft Publishers CY - Sofia ER - TY - JOUR A1 - Hubrig, Swetlana A1 - Schöller, Markus A1 - Kholtygin, Alexander F. A1 - Tsumura, Hiroki A1 - Hoshino, Akio A1 - Kitamoto, Shunji A1 - Oskinova, Lida A1 - Ignace, Richard A1 - Todt, Helge Tobias A1 - Ilyin, Ilya T1 - New multiwavelength observations of the Of?p star CPD-28 degrees 2561 JF - Monthly notices of the Royal Astronomical Society N2 - A rather strong mean longitudinal magnetic field of the order of a few hundred gauss was detected a few years ago in the Of?p star CPD -28 degrees 2561 using FORS2 (FOcal Reducer low dispersion Spectrograph 2) low-resolution spectropolarimetric observations. In this work, we present additional low-resolution spectropolarimetric observations obtained during several weeks in 2013 December using FORS 2 mounted at the 8-m Antu telescope of the Very Large Telescope (VLT). These observations cover a little less than half of the stellar rotation period of 73.41 d mentioned in the literature. The behaviour of the mean longitudinal magnetic field is consistent with the assumption of a single-wave variation during the stellar rotation cycle, indicating a dominant dipolar contribution to the magnetic field topology. The estimated polar strength of the surface dipole B-d is larger than 1.15 kG. Further, we compared the behaviour of the line profiles of various elements at different rotation phases associated with different magnetic field strengths. The strongest contribution of the emission component is observed at the phases when the magnetic field shows a negative or positive extremum. The comparison of the spectral behaviour of CPD -28 degrees 2561 with that of another Of?p star, HD 148937 of similar spectral type, reveals remarkable differences in the degree of variability between both stars. Finally, we present new X-ray observations obtained with the Suzaku X-ray Observatory. We report that the star is X-ray bright with log L-X/L-bol approximate to -5.7. The low-resolution X-ray spectra reveal the presence of a plasma heated up to 24 MK. We associate the 24 MK plasma in CPD -28 degrees 2561 with the presence of a kG strong magnetic field capable to confine stellar wind. KW - stars: atmospheres KW - stars: individual: CPD-28 degrees 2561 KW - stars: magnetic field KW - stars: mass-loss KW - stars: variables: general KW - X-rays: stars Y1 - 2015 U6 - https://doi.org/10.1093/mnras/stu2516 SN - 0035-8711 SN - 1365-2966 VL - 447 IS - 2 SP - 1885 EP - 1894 PB - Oxford Univ. Press CY - Oxford ER - TY - JOUR A1 - Schöller, Markus A1 - Hubrig, Swetlana A1 - Fossati, L. A1 - Carroll, Thorsten Anthony A1 - Briquet, Maryline A1 - Oskinova, Lida A1 - Järvinen, S. A1 - Ilyin, Ilya A1 - Castro, N. A1 - Morel, T. A1 - Langer, N. A1 - Przybilla, N. A1 - Nieva, M. -F. A1 - Kholtygin, A. F. A1 - Sana, H. A1 - Herrero, A. A1 - Barba, R. H. A1 - de Koter, A. T1 - B fields in OB stars (BOB) BT - Concluding the FORS2 observing campaign JF - Astronomy and astrophysics : an international weekly journal N2 - Aims. The B fields in OB stars (BOB) Collaboration is based on an ESO Large Programme to study the occurrence rate, properties, and ultimately the origin of magnetic fields in massive stars. Methods. In the framework of this program, we carried out low-resolution spectropolarimetric observations of a large sample of massive stars using FORS2 installed at the ESO VLT 8m telescope. Results. We determined the magnetic field values with two completely independent reduction and analysis pipelines. Our in-depth study of the magnetic field measurements shows that differences between our two pipelines are usually well within 3 sigma errors. From the 32 observations of 28 OB stars, we were able to monitor the magnetic fields in CPD -57 degrees 3509 and HD164492C, confirm the magnetic field in HD54879, and detect a magnetic field in CPD -62 degrees 2124. We obtain a magnetic field detection rate of 6 +/- 3% for the full sample of 69 OB stars observed with FORS 2 within the BOB program. For the preselected objects with a nu sin i below 60 km s(-1), we obtain a magnetic field detection rate of 5 +/- 5%. We also discuss X-ray properties and multiplicity of the objects in our FORS2 sample with respect to the magnetic field detections. KW - polarization KW - stars: early-type KW - stars: magnetic field KW - stars: massive Y1 - 2017 U6 - https://doi.org/10.1051/0004-6361/201628905 SN - 1432-0746 VL - 599 PB - EDP Sciences CY - Les Ulis ER - TY - GEN A1 - Morel, T. A1 - Castro, Norberto A1 - Fossati, Luca A1 - Hubrig, Swetlana A1 - Langer, N. A1 - Przybilla, Norbert A1 - Schöller, Markus A1 - Carroll, Thorsten Anthony A1 - Ilyin, Ilya A1 - Irrgang, Andreas A1 - Oskinova, Lida A1 - Schneider, Fabian R. N. A1 - Simon Díaz, Sergio A1 - Briquet, Maryline A1 - González, Jean-Francois A1 - Kharchenko, Nina A1 - Nieva, M.-F. A1 - Scholz, Ralf-Dieter A1 - de Koter, Alexander A1 - Hamann, Wolf-Rainer A1 - Herrero, Artemio A1 - Maíz Apellániz, Jesus A1 - Sana, Hugues A1 - Arlt, Rainer A1 - Barbá, Rodolfo H. A1 - Dufton, Polly A1 - Kholtygin, Alexander A1 - Mathys, Gautier A1 - Piskunov, Anatoly E. A1 - Reisenegger, Andreas A1 - Spruit, H. A1 - Yoon, S.-C. T1 - The B fields in OB stars (BOB) survey T2 - Postprints der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe N2 - The B fields in OB stars (BOB) survey is an ESO large programme collecting spectropolarimetric observations for a large number of early-type stars in order to study the occurrence rate, properties, and ultimately the origin of magnetic fields in massive stars. As of July 2014, a total of 98 objects were observed over 20 nights with FORS2 and HARPSpol. Our preliminary results indicate that the fraction of magnetic OB stars with an organised, detectable field is low. This conclusion, now independently reached by two different surveys, has profound implications for any theoretical model attempting to explain the field formation in these objects. We discuss in this contribution some important issues addressed by our observations (e.g., the lower bound of the field strength) and the discovery of some remarkable objects. T3 - Zweitveröffentlichungen der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe - 821 KW - magnetic fields KW - stars: early-type KW - stars: magnetic fields KW - stars: individual (HD 164492C, CPD –57 ◦ 3509, HD 54879, β CMa, ε CMa) Y1 - 2020 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-415238 SN - 1866-8372 IS - 821 ER -