Massive Star Formation
Dense molecular cocoons in the massive protocluster W3 IRS5: a test case for models of massive star formation
... of massive star formation has been made recently with at centimeter, and (sub)millimeter ...of star formation as proposed by Bonnell et ...turbulent, massive star-forming ...
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Sokolov, Vlas (2018): Early stages of massive star formation. Dissertation, LMU München: Fakultät für Physik
... of star and planet formation, providing sensitivity enough to image young protostars and protoplanetary systems with an angular resolution comparable to that of ...In massive star ...
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The Location, Clustering, and Propagation of Massive Star Formation in Giant Molecular Clouds
... of massive star formation and its relation with GMCs in the Large Magellanic Cloud ( LMC ) ...the formation of massive stars in a wide range of evolutionary stages, since its face-on ...
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Observational signatures of massive star formation : an investigation of the environments in which they form, and the applicability of the paradigm of low mass star formation
... of massive stars with disks given in Cesaroni et ...more massive than their low-mass counterparts (see Section ...more massive protostars, whose accretion timescales are commonly smaller than their ...
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Constraints on massive star formation: Cygnus OB2 was always an association
... very massive stars, including at least two stars as massive as ∼ 100 M # , this allows us to constrain the sites and conditions under which massive stars ...The formation of these ...
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Early-stage Massive Star Formation near the Galactic Centre: Sgr C
... mass star formation in the Sgr C cloud was reported by Forster & Caswell (2000), who detected a faint 8–9 GHz radio source measuring ...mass star formation and outflows (De Buizer & ...
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RCW36: characterizing the outcome of massive star formation
... a massive star is identified as the source of ionizing radiation that formed the ultra-compact H region (UCHII, ...sequential star formation. In other cases, star formation ...
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Multi-generation massive star-formation in NGC 3576
... central star cluster have uncovered evidence of sequential star- formation leading us to believe that the adjacent clumps may host massive protostellar objects at a very early stage of ...
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The VLT-FLAMES Tarantula Survey III. A very massive star in apparent isolation from the massive cluster R136
... halt and reverse the accretion flow onto the central object (e.g. Yorke & Kruegel 1977). However, recent multi-dimensional hy- drodynamical monolithic collapse simulations indicate that mas- sive stars may form via ...
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Joint Astrophysics Nascent Universe Satellite:. utilizing GRBs as high redshift probes
... the massive star formation rate over 5 ≤ z ≤ 12 by discovering and observing high-z gamma-ray bursts (GRBs) and their afterglows, (2) enable detailed studies of the history of reionization and metal ...
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Trajectories of bright stars at the Galactic Center as a tool to evaluate a graviton mass
... cluding massive graviton theories introduced by Fierz and Pauli [30] are a subject of intensive ...of massive graviton a gravitational wave signal is di ff erent from a signal of general relativity [31, ...
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The standard model of low-mass star formation applied to massive stars: multiwavelength modelling of IRAS 20126+4104
... best-fitting values of the remaining parameters are given in Table 3. Our results show that the envelope plus disc model reproduces the observed SED and images better than the envelope without disc model, although the ...
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The standard model of low-mass star formation applied to massive stars: a multi-wavelength picture of AFGL 2591
... Evidence for the presence of a disk or rotationally flattened material around the central source of AFGL 2591 has been found by several authors. The near-IR imaging polarimetry observa- tions of Minchin et al. (1991) ...
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A 'super' star cluster grown old: the most massive star cluster in the Local Group
... Subsequently, we placed the origin and early evolution of this M31 GC in the context of the YMCs currently being observed in ma- jor starbursts and galaxy mergers in the local Universe. 037−B327 is a prime example of an ...
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Pfuhl, Oliver (2012): The GRAVITY interferometer and the Milky Way’s nuclear star cluster. Dissertation, LMU München: Fakultät für Physik
... In terms of mass, the resolved stellar population represents only the tip of the iceberg. The bulk of the stellar mass is unresolved. Therefore the diffuse background emission of the GC contains valuable information on ...
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Simultaneous low and high mass star formation in a massive protocluster : ALMA observations of G11 92 0 61
... regions of the IRDC G11.11-0.12 P6 by Wang et al. 2014). Estimates of the total mass in compact cores—e.g. includ- ing the previously-known sources MM1, MM2, and MM3– depend on the mass estimates for these sources, which ...
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A detailed study of feedback from a massive star
... OB star is of the order of 10 ...companion star or stellar ...very massive low-metallicity stars undergoing direct collapse to a black hole, many with a weak or no ...
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Young massive star cluster formation in the Galactic Centre is driven by global gravitational collapse of high-mass molecular clouds
... for star formation, which appear to accurately predict the star formation rate for Galactic Disc star-forming regions, (Lada et ...
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Gobat, Raphael (2009): Evolution of early-type galaxies in field and cluster environments at z~1. Dissertation, LMU München: Fakultät für Physik
... erarchical formation scenario. For this reason, modern models of galaxy formation and evolution are based on this latter ...where star formation is regulated by internal processes, such as the ...
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On the massive stellar population of the super star cluster Westerlund 1
... more massive than R136 and at least comparable to (and probably more massive than) the NGC 2070 cluster at the heart of the 30 Dor ...host massive stellar ...O star census is unlikely to ...
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