Interstellar Medium and Star formation
Dusty super star cluster winds: their impact on the interstellar medium and infrared manifestations
... radiative and mechanical feedback on the interstellar medium ...radiation and thus are powerful diagnostic tool to study star formation as well as the chemical composition of ...
113
Evolution of star-forming dwarf galaxies: characterizing the star formation scenarios
... gasping and bursting ...SF and the bursting scenario (Marconi et ...gasping and bursting scenarios is that short episodes of SF enrich the interstellar medium (ISM) in a time-scale of ...
15
Evolution of star-forming dwarf galaxies: characterizing the star formation scenarios
... gasping and bursting ...SF and the bursting scenario (Marconi et ...gasping and bursting scenarios is that short episodes of SF enrich the interstellar medium (ISM) in a time-scale of ...
15
Biomolecules and interstellar molecules: structure, interactions and spectroscopic characterization
... the interstellar medium due to the ongoing astronomical observations complemented with elaborated laboratory ...abundant interstellar elements H, C, N, and O and are found mainly in the ...
304
On the extreme positive star formation feedback condition in scuba sources
... winds and supernovae explosions in young assembling ...plasma, and the gravitational pull of the host galaxy lead to three different hydrodynamic ...zones and gas expulsion from the outer zones of ...
7
A Study of Two Dwarf Irregular Galaxies with Asymmetrical Star Formation Distributions
... compact star clusters in the LEGUS sample of galaxies ( Adamo et ...3738, and we use the LEGUS catalog to examine the star clusters in each half of the ...compact and centrally concentrated ...
13
Observational evidence of star formation stochasticity in the CALIFA dataset
... stars and the die that is thrown many times is a region of high ...a star forming locality has a high SFR, sampling the IMF is ...[3] and thus the IMF is not completely ...luminosity and ...
36
INTERSTELLAR ABSORPTION TOWARDS THE NOVAE V339 DEL AND V5668 SGR
... Small and Large Magellanic Clouds (Vladilo et ...useful and distant back- ground light sources are extragalactic supernovae (SN) (D’Odorico et ...the interstellar absorption in our Galaxy and ...
9
Herschel ATLAS: The cosmic star formation history of quasar host galaxies?
... pixel, and zero everywhere ...far-infrared and submm ...mass and the companion galaxies may in time be accreted by the QSO host ...the star formation inferred from the flux in the ...
5
STAR FORMATION RATE IN LATE-TYPE GALAXIES: I- THE Hα AND FUV INTEGRATED VALUES
... values and those reported by Lee et al. (2009) and Hunter & Elmegreen (2004), with the latter authors using the color excess and the extincion law of Cardelli et ...(1989) and the former ...
16
Multiwavelength Study of Massive Galaxies at z~2 I Star Formation and Galaxy Growth
... between star formation tracers as calibrated locally and based on the radio, far-IR, mid-IR, and even UV (cor- rected for the extinction by dust) and the ...Herschel, and later ...
17
Recent Galaxy Mergers and Residual Star Formation of Red Sequence Galaxies in Galaxy Clusters
... features, and they mostly populated the less massive end of the sample ’ s mass range ( - 21 M r ¢ < - 20 ) ...) and the young stellar populations (∼ 1 Gyr ) , the fraction of RSF red sequence galaxies ...
9
(gamma)-ray emission from regions of star formation: Theory and observations with the MAGIC Telescope
... NSB and, therefore, may change the shape of the recorded ...thresholds, and different general performance of the ...June and November 2005, in order to check for the necessity of using different MC ...
259
Interactions, star formation and extended nebulae in SDSS type 2 quasars at 0.3 ≲ z ≲ 0.6.?
... metallicities and they also seem specially prevalent in quasars showing signs of strong galaxy interactions ...ulae and characterizing their general ...quiet and have large nuclear line ...
17
Simulations of star formation in a gaseous disc around Sgr A* a failed Active Galactic Nucleus
... For longer cooling times, that is, β 1, disc fragmentation is less vigorous, creating fewer stars and leading to a more top-heavy IMF. In this case, while the gaseous mass is still comparable to the stellar mass ...
13
The formation of dwarf spheroidal galaxies including their star formation histories La formación de galaxias esferoidales enanas incluyendo sus historias de formación estelar
... surviving star cluster, even though 30% is close to the theoretical ...survive and that is in the very center of a cored DM ...orbit and so we see SC remnants, especially if the SC is close to its ...
80
Strategic resilience and crises in small and medium enterprises
... changes and innovate and thus find the elements that help small and medium enterprises to get ahead and in the best case of a strengthened ...
12
Luminosity functions of local infrared galaxies with AKARI : implications for the cosmic star formation history and AGN evolution
... 22 and 24 µ m using the AKARI photometry at 9 and 18 µ m, and the best-fitting CHEL model from Section ...precise and easily reproducible definitions of monochromatic luminosity, we chose such ...
12
Panchromatic estimation of star formation rates in BzK galaxies at 1 <z< 3
... 1.2 and a cutoff energy of 20 ...galaxies and soft X-ray selected ...flux and luminosity conversions using Γ = ...nosities, and SFRs are tabulated in Table 7 and discussed in Section ...
15
LOW AND MEDIUM VOLTAGE FOR HAZARDOUS AREAS
... mixture and it avoids such explosion to go out from this enclosure to an external explosive ...in and out. While the motor is in operation, it heats up and the internal air gets to a higher pressure ...
36
