[PDF] Top 20 Water in star-forming regions with Herschel (WISH). V. The physical conditions in low-mass protostellar outflows revealed by multi-transition water observations
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Water in star-forming regions with Herschel (WISH). V. The physical conditions in low-mass protostellar outflows revealed by multi-transition water observations
... shock conditions are such that a C-type shock does not have time to reach steady-state; in this case, a J-type front develops at the time the shock is truncated (Chieze et ...different conditions or ... See full document
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Linking low- to high-mass young stellar objects with Herschel-HIFI observations of water
... In Star-forming regions with Herschel” key programme (WISH; van Dishoeck et ...several water lines, as well as high- J CO and isotopologue transitions, for a large sample of YSOs ... See full document
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Herschel-HIFI observations of high-J CO and isotopologues in star-forming regions: from low to high mass
... erent regions of the proto- stellar environment with different physical ...logue transition are presented in ...of protostellar envelopes, characterise the turbulence in the envelope-outflow ... See full document
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Unveiling the Physical Conditions in Star-Forming Galaxies at the Peak of Galaxy Assembly
... in low-density ionized gas, as they are able to convert kinetic energy in the gas into electromagnetic emission through collisionally-excited ...II regions with maximal values of R23( ≈ ... See full document
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Comparisons between different techniques for measuring mass segregation
... and low-mass stars. Therefore the dis- tribution of low-mass stars must be known, however these are very faint compared to the high-mass stars in young re- ...observing ... See full document
14
Trigonometric Parallaxes of High-mass Star-forming Regions: Our View of the Milky Way
... The locations of the maser stars listed in Table 1 projected onto the Galactic plane are shown in Fig. 1 superposed on a schematic plot of the Milky Way as viewed from the north Galactic pole where rotation is clockwise. ... See full document
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Alignment between Protostellar Outflows and Filamentary Structure
... filaments forming due to converging flows, mass flows along mag- netic field lines to both the filaments and cores (which form ...some observations have suggested that magnetic field lines are ... See full document
18
Distributed star formation throughout the galactic center cloud Sgr B2
... The relative ages of M and the rest of the region (i.e., Sgr B2 M is apparently older) suggest two possibilities for their formation history. If we take the ages at face value, Sgr B2 M must have collapsed first to form ... See full document
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Dynamical evolution of star-forming regions
... system mass segregates, although this needs to be tested fully as all simulations have so far neglected binaries ...system mass, massive star binaries could in principle facilitate a higher degree of ... See full document
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Infall Signatures in a Prestellar Core Embedded in the High-mass 70 μm Dark IRDC G331.372-00.116
... the mass of the core, making the scenario observed in IRDC ...its mass over time to eventually gather sufficient mass to form a high-mass ... See full document
13
Modelling high resolution ALMA observations of strongly lensed highly star forming galaxies detected by Herschel
... the Herschel Space Observatory. Our modelling recovers mass properties of the lensing galaxies and, by determining magnification factors, in- trinsic properties of the lensed sub-millimetre ...of ... See full document
13
Modelling high-resolution ALMA observations of strongly lensed highly star-forming galaxies detected by Herschel
... power-law mass den- sity profile, we find that the lenses are all close to isothermal and that the recovered model parameters are in broad agree- ment between both ...dust mass, luminos- ity and inferred ... See full document
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Water distribution in shocked regions of the NGC 1333-IRAS 4A protostellar outflow
... the water distribution around ...different water kinematic compo- nents mentioned above (see ...in water line profiles offset from the shock position, which show a triangular wing ...the water ... See full document
12
The low mass content of the massive young star cluster RCW 38
... lowest mass bins have been corrected for incompleteness, according to the average Ks-band magnitude of the sources belonging to it, and the curve shown in ...lowest mass bins, where the correction is ... See full document
14
The Depletion of Water During Dispersal of Planet-forming Disk Regions
... spectral resolution of observing techniques. Direct imaging is able to reveal gap sizes ( if their angular size is large enough to be spatially resolved ) and the relative distribution of dust grain populations ( small ... See full document
23
The SFR-M* Relation and Empirical Star-Formation Histories from ZFOURGE at 0.5 < z < 4
... stellar mass, we use two techniques to extract empirical star formation and mass growth histories from observations ( see Figure 11 ) ...initial conditions. The second technique ... See full document
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Interaction between karstic aquifers and allogenic rivers: The aquifer of the national park of the ephemeral river Lobos Canyon (Spain)
... that water flows out of the system via Ucero. In dry weather (low water) periods, and in the lower reaches, the water table comes to the surface in the deep pools (which assume great ... See full document
17
Multi-wavelength de-blended Herschel view of the statistical properties of dusty star-forming galaxies across cosmic time
... metal mass is in dust grains and a Zubko et ...HII regions, and temperature thresh- old for is set in order to reproduce FIR properties of the local galaxies in the Herschel Reference Survey (Boselli ... See full document
21
Spitzer catalog of Herschel selected ultrared dusty, star forming galaxies
... end of our sample. Since leaving redshift as a free pa- rameter introduces extra degree of freedom and degen- eracy in SED fitting than fixing the redshift, here we also compare with the magphys results by fixing the in- ... See full document
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There is no magnetic braking catastrophe : low mass star cluster and protostellar disc formation with non ideal magnetohydrodynamics
... The calculations we present here extend the investigation of magnetized star formation in two main ways beyond the studies mentioned above. First, they are the first calculations of the forma- tion of stellar ... See full document
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