[PDF] Top 20 Star formation in Galactic flows
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Star formation in Galactic flows
... of star forma- tion from galactic scale ...in star for- mation over a ...subsequent star formation in the dense ridge of gas thus ...the star formation from the point of ... See full document
8
The formation of the Galactic bulge of the Milky Way
... Abstract. We aim to determine if the bulge formed via mergers as predicted by Cold Dark Matter (CDM) theory, or from disk instabilities, as suggested by its boxy shape, or both processes. We are observing about 28,000 ... See full document
5
ALMA observations of a $z$ ≈ 3.1 Protocluster: Star Formation from Active Galactic Nuclei and Lyman-Alpha Blobs in an Overdense Environment
... and star formation and the various tight relationships between BH mass and the properties of nearby galaxies ...of star formation per galaxy in the SSA 22 ... See full document
11
Astrophysical site(s) of r-process elements in galactic chemodynamical evolution model
... lower star for- mation efficiency in smaller mass sub-haloes ...galaxy formation also suggest that it is possible to reproduce the observation by NSMs with merger time of 100 Myr [22, ... See full document
7
The formation history of the Galactic bulge
... of star formation. Solar values are achieved when extended star formation takes place, so that the debris from SNeIa can be incorporated into subsequent generations of ...low star ... See full document
11
A Magnified View of Circumnuclear Star Formation and Feedback around an Active Galactic Nucleus at z=2 6
... active galactic nuclei ( AGNs ) , are thought to regulate the growth of the surrounding stellar bulge through energy and momentum return into the interstellar medium ( ISM; see Fabian 2012 for a review ) ... See full document
7
Chemical constraints on the formation of the Galactic thick disk
... the Galactic disk, and the degree of the separation between the two disks, we have undertaken a large spectroscopic survey of F and G dwarf stars in the Solar ...the formation history of the Milky Way, and ... See full document
7
The coordinated radio and infrared survey for high-mass star formation - IV. A new radio-selected sample of compact galactic planetary nebulae
... the number of known PNe, it is important that PNe are searched for at longer wavelengths. The CORNISH observations at 6 cm provides us with a sample of PNe that is not affected by extinction. The reliability of this ... See full document
27
OMEGA – OSIRIS Mapping of Emission line Galaxies in A901/2: II Environmental influence on integrated star formation properties and AGN activity
... diagram: star-forming galaxies, strong AGN (sAGN) or Seyferts, weak AGN (wAGN) or LINERs and the so- called retired galaxy population (Cid Fernandes et ...the galactic disc ... See full document
18
The dynamics and star-forming potential of the massive Galactic centre cloud G0.253+0.016
... the star formation column density threshold for ...the Galactic disk, yet incorpo- rating turbulence might still not account for the lack of mas- sive star formation ...for star ... See full document
19
Gobat, Raphael (2009): Evolution of early-type galaxies in field and cluster environments at z~1. Dissertation, LMU München: Fakultät für Physik
... the formation and evolution of galaxies is still one of the great questions in cosmology, more than eighty years after galaxies were recognized for what they are, “island universes” of their own rather than mere ... See full document
161
The mean star formation rates of unobscured QSOs: searching for evidence of suppressed or enhanced star formation
... ing QSO samples the optical–ultraviolet (UV) is no longer an option for determining the star formation as the QSO light dominates at these wavelengths. We use FIR data from the Herschel-ATLAS (H-ATLAS) ... See full document
20
Pfuhl, Oliver (2012): The GRAVITY interferometer and the Milky Way’s nuclear star cluster. Dissertation, LMU München: Fakultät für Physik
... reduced star formation, while during the last few 100 Myrs the star formation rate was ...The formation of the cluster might coincide with the formation of the bulge around 10 ± ... See full document
169
Kiloparsec-scale Simulations of Star Formation in Disk Galaxies. IV. Regulation of Galactic Star Formation Rates by Stellar Feedback
... their star formation activity that result from different implementations of feedback ...massive star clusters form in the no-feedback run, while these are mostly dispersed during the sequence LW, LW ... See full document
24
Submillimeter evidence for the coeval growth of massive black holes and galaxy bulges
... active galactic nuclei (AGN) by accretion of the same gas that is rapidly forming the stars which make up the spheroid, ...the formation of the spheroid and the growth of the massive black hole are ... See full document
8
GASTON: Galactic Star Formation with NIKA2 A new population of cold massive sources discovered
... erent star formation regimes for every part of the IMF where the power-law slope ...the formation of low-mass stars inside them [3, ...the formation of cores more massive than a few solar ... See full document
6
Galaxy Formation and Chemical Evolution
... the formation of the earliest generations of stars is considered to have commenced quite ...the galactic inventories of all the stable nuclides ...the star formation rate at different epochs ... See full document
9
Early-stage Massive Star Formation near the Galactic Centre: Sgr C
... three star-forming cores in the EGO contrasts with the absence of further star formation in the host molecular cloud, placing Sgr C at an interesting mid-point between the quiescent ... See full document
6
Class I methanol masers in NGC253: alcohol at the end of the bar
... some Galactic methanol masers have been demonstrated to have the emission from the ...studied Galactic methanol maser transi- ...strongest Galactic sources and so there appears little prospect of ... See full document
12
Influence of Supernova SN Ia Rate and the Early Star Formation Rate on the Galactic Chemical Evolution
... the formation of successive generations of stars in a discrete manner compared to the other GCE models developed earlier that are based on the averaged evolutionary behavior of the galaxy [3-6], the normalized SN ... See full document
9
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