Zobrazeno 1 - 10
of 252
pro vyhledávání: '"Altenburg, J."'
Autor:
Pflamm-Altenburg, J., Kroupa, P., Thies, I., Jerabkova, T., Beccari, G., Prusti, T., Boffin, H. M. J.
Publikováno v:
A&A 671, A88 (2023)
Context: Tidal tails of star clusters are commonly understood to be populated symmetrically. Recently, the analysis of Gaia data revealed large asymmetries between the leading and trailing tidal tail arms of the four open star clusters Hyades, Praese
Externí odkaz:
http://arxiv.org/abs/2301.02251
Autor:
Akkerman, O.W., Altenburg, J., Bakker, M., Bannier, M.A.G.E., Conemans, L.H., Gulmans, V.A.M., Heijerman, H.G.M., Hoek, R.A.S., Janssens, H.M., van der Meer, R., Merkus, P.J.F.M., Noordhoek, J.J., Nuijsink, M., Terheggen-Lagro, S.W.J., van der Vaart, H., de Winter-de Groot, K.M., Zomer, Domenique, van Ingen, Jakko, Hofland, Regina
Publikováno v:
In Journal of Cystic Fibrosis March 2023 22(2):327-333
Autor:
Terpstra, L.C., Altenburg, J., Bronsveld, I., Doodeman, H.J., Rozemeijer, W., Heijerman, H.G.M., Boersma, W.G.
Publikováno v:
In Contemporary Clinical Trials Communications December 2022 30
Publikováno v:
A&A 594, A119 (2016)
Ultra-compact dwarf galaxies (UCDs) share many properties with globular clusters (GCs) and are found in similar environments. A large sample of UCDs and GCs around NGC 1399, the central giant elliptical of the Fornax galaxy cluster, is used to infer
Externí odkaz:
http://arxiv.org/abs/1607.06443
Autor:
Kim Elsink, Manon M. H. Huibers, Iris H. I. M. Hollink, Annet Simons, Evelien Zonneveld-Huijssoon, Lars T. van der Veken, Helen L. Leavis, Stefanie S. V. Henriet, Marcel van Deuren, Frank L. van de Veerdonk, Judith Potjewijd, Dagmar Berghuis, Virgil A. S. H. Dalm, Clementien L. Vermont, Annick A. J. M. van de Ven, Annechien J. A. Lambeck, Kristin M. Abbott, P. Martin van Hagen, Godelieve J. de Bree, Taco W. Kuijpers, Geert W. J. Frederix, Mariëlle E. van Gijn, Joris M. van Montfrans, the Genetics First for Primary Immunodeficiency Disorders Consortium, Aerde van, KJ, Altenburg, J, Armbrust W, Barendregt, BH, Berg van den, JM, Bredius, RGM, Buddingh, EP, Burg van der, M, Ellerbroek, PM, Ernst, RF, Fraaij, PLA, Hermans, M, Hoischen, A, Hout van der, AH, Jansen, MHA, Jolink, H, Jonkers, RE, Laar van, JAM, Leeuw de, K, Legger, GE, Leijten, EFA, Limper, M, Lindemans, CA, Oever ten, J, Pieterse, M, Rombach, SM, Rossum van, AMC, Rutgers, A, Santen, GWE, Schölvinck, EH, Simon, A, Stol, K, Vervenne RML
Publikováno v:
Frontiers in Immunology, Vol 12 (2021)
ObjectiveInborn errors of immunity (IEI) are a heterogeneous group of disorders, affecting different components of the immune system. Over 450 IEI related genes have been identified, with new genes continually being recognized. This makes the early a
Externí odkaz:
https://doaj.org/article/1589a20c7b90482f8384cabc050aeb63
A significant fraction of massive stars in the Milky Way and other galaxies are located far from star clusters. It is known that some of these stars are runaways and therefore most likely were formed in embedded clusters and then ejected into the fie
Externí odkaz:
http://arxiv.org/abs/1206.1596
It has been known for a long time that the satellite galaxies of the Milky Way (MW) show a significant amount of phase-space correlation, they are distributed in a highly inclined Disc of Satellites (DoS). We have extended the previous studies on the
Externí odkaz:
http://arxiv.org/abs/1204.5176
Direct N-body calculations are presented of the early evolution of exposed clusters to quantify the influence of gas expulsion on the time-varying surface brightness. By assuming that the embedded OB stars drive out most of the gas after a given time
Externí odkaz:
http://arxiv.org/abs/1112.1068
Using archival Spitzer Space Telescope data, we identified for the first time a dozen runaway OB stars in the Small Magellanic Cloud (SMC) through the detection of their bow shocks. The geometry of detected bow shocks allows us to infer the direction
Externí odkaz:
http://arxiv.org/abs/1010.2490
The origin of massive field stars in the Large Magellanic Cloud (LMC) has long been an enigma. The recent measurements of large offsets (~100 km/s) between the heliocentric radial velocities of some very massive (O2-type) field stars and the systemic
Externí odkaz:
http://arxiv.org/abs/1006.0225