Magellanic Clouds
The Relationship Between Molecular Gas, H I, and Star Formation in the Low-mass, Low-metallicity Magellanic Clouds
... nearby Magellanic Clouds, we are in a unique position to probe how the relationship between the molecular gas and star formation rate behave as a function of metallicity and the size scale ...
24
Results of the ESO-SEST Key Programme on CO in the Magellanic Clouds. X. CO emission from star formation regions in LMC and SMC
... the Magellanic Clouds. It was noted that the Magellanic Clouds allow investigation ofmolecular gas and cloud complexes un- der conditions of low metallicity and high radiation densities as ...
12
Results of the ESO-SEST key programme: CO in the Magellanic Clouds. VI. The 30 DOR Complex
... molecular clouds, we rely on millimeter wave observations of carbon monoxide (CO), a trace con- ...molecular clouds to their masses has been a topic of considerable ...of clouds. In the ...
12
Sasaki, Manami (2002): X-rays tracing the star formation history of the Magellanic clouds. Dissertation, LMU München: Fakultät für Physik
... the Magellanic Clouds has been ...the Magellanic Clouds in the soft X-ray band and by analyzing the hot component of the interstellar ...
175
The Master Catalogue of stars towards the Magellanic Clouds. I. Multispectral surveys of the Large Magellanic Cloud
... The Magellanic Clouds (MCs) are among the best suitable places to study the stellar evolution outside the Milky Way, because of their proximity and their various stellar popula- ...The Magellanic ...
13
Results of the SEST Key Programme: CO in the Magellanic Clouds. VIII. The giant molecular complex No. 37 of the LMC
... morphology and velocity structure within each cloud. For instance, cloud C exhibits two peaks separated by ∼ 1. 0 2. The observed spatial-velocity distribution does not, how- ever, indicate the presence of two distinct, ...
16
A Spectroscopic Study of Planetary Nebulae in the Magellanic Clouds
... A recent analysis of an ultraviolet spectrum of this object (Barlow et 0/., 1986) estimates the ratio of the total stellar flux (including emission features) to the continuum f[r] ...
183
An infrared study of the Magellanic clouds
... d) The Clouds' flux densities at the distance of the M81-group and the Virgo cluster are given. Limits for detection of sources with the same infrared flux density as the Clouds are also[r] ...
297
Properties of Anomalous and Type II Cepheids in the Small and Large Magellanic Clouds
... Abstract. The Small Magellanic Cloud (SMC) and Large Magellanic Cloud (LMC) give us the possibility to study individual variable star types in a new way. Literature data provide us with photometric ...
5
Surveys of the Milky Way and Magellanic System in the λ21-cm line of atomic hydrogen
... the Magellanic Clouds and Stream in both emission and absorption in the H I 21-cm line and the OH 18-cm ...cool clouds. Tracing turbulence in the Magellanic Stream shows how extra-galactic gas ...
6
Chemical abundances in the Leading Arm of the Magellanic Stream
... Our second observation is that there is spatial variation of the oxygen abundances. The two directions through region LA III have identical (low) oxygen abundances, given the observa- tional errors, with [O/H] = − ...
15
Multiwavelength observations of nova SMCN 2016 10a one of the brightest novae ever observed
... Small Magellanic Cloud (SMC) occur less ...the Magellanic Clouds, offering a systematic study of novae in the SMC where they derived an observed rate of ...
31
Old star clusters: Bench tests of low mass stellar models
... Here it is adopted the ‘evolutionary’ definition of ‘old’, i.e. clusters are denoted as ‘old’ when they are populated by stars that produce an electron degenerate He-core at the end of the Main Sequence (MS). In terms of ...
9
Grimm, Hans-Jakob (2003): X-ray binaries in the Milky Way and other galaxies. Dissertation, LMU München: Fakultät für Physik
... Based on CHANDRA and ASCA observations of nearby star forming galaxies and RXTE/ASM, ASCA, and MIR- KVANT/TTM data on our Galaxy and the Magellanic Clouds we studied the relation between[r] ...
128
Infrared composition of the Large Magellanic Cloud
... With Spitzer it became possible to obtain 5–40 μm spec- troscopy of many point sources in the LMC and SMC. In- deed, many observing programs were proposed, some tar- geting just a single or a few point sources, while ...
5
The Draco dwarf galaxy in the near-infrared
... 3.1.3. 4) shows no clear-cut separation between sources of a di ff erent type as was the case for the Magellanic Clouds (Cioni et al. Only two known carbon stars seem to fall within the e[r] ...
12
Numerical simulations of a shock interacting with multiple magnetized clouds
... multiple clouds, and attempts to lay some of the necessary foundations for understanding this ...spherical clouds, which could significantly change the forces acting on the ...between clouds whose ...
24
Detecting cloud contamination in passive microwave satellite measurements over land
... all clouds seen by vis–IR measurements, especially when only a subset of the frequencies is ...thin clouds, high semi- transparent meanly thick clouds, and the fractional clouds ...the ...
13
Technology Futures for ACES: Clouds Web2 0 and Multicore
... Clouds can be built from Grids but will hide this from user Clouds designed to build 100 times larger data centers Clouds support green computing by supporting remote location where oper[r] ...
29
Introduction to Clouds and the VSCSE Summer School on Science Clouds
... • Several Applications with 3 talks on Life Sciences and talks on experiences with HPC on the cloud and use of specific technologies in particular applications • Virtual Machine manageme[r] ...
69