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[PDF] Top 20 Class II methanol masers and their environment at high resolution

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Class II methanol masers and their environment at high resolution

Class II methanol masers and their environment at high resolution

... The main ATCA observations consist of the 6.7-GHz surveys by Caswell, mentioned above, observations of the 6.7-GHz maser emission and absorption in the molecular cloud complex Sgr B2 Hou[r] ... See full document

183

HiReD: a high-resolution multi-window visualisation environment for cluster-driven displays

HiReD: a high-resolution multi-window visualisation environment for cluster-driven displays

... the High-Resolution Desktop (HiReD), an extendable multi-window environment designed for performing interac- tive visual data ...ate high-resolution data visualisations and makes use of ... See full document

11

6 7 GHz maser astrometry with the Australian long baseline array

6 7 GHz maser astrometry with the Australian long baseline array

... as masers. Astrophysical masers are prominent, point–like radio sources, which are associated with interstellar and stellar sources, as well as with galactic nuclei, comets and ...interstellar masers ... See full document

183

The extraordinary outburst in the massive protostellar system NGC6334I MM1 : emergence of strong 6 7 GHz methanol masers

The extraordinary outburst in the massive protostellar system NGC6334I MM1 : emergence of strong 6 7 GHz methanol masers

... central environment of a massive star- forming region. We have obtained high resolution (∼500 au) VLA images of multiple maser transitions which reveal the first appearance of Class II ... See full document

17

High mass star formation in the nearby region G352 630 1 067  I  parallax

High mass star formation in the nearby region G352 630 1 067 I parallax

... generate high-mass ...isolated environment than others, hence providing an excellent candidate for investigations of the processes that form individual high-mass ...GHz methanol maser and ... See full document

11

A new 95GHz methanol maser catalog  I  Data

A new 95GHz methanol maser catalog I Data

... methanol masers, but not as ef fi cient as EGO-based search criteria ( ...with class  I methanol masers is not surprising; however, the detection rate achieved toward the current BGPS ... See full document

12

High resolution radar for automobile applications

High resolution radar for automobile applications

... with high res- olution in range and azimuth generating real-aperture radar images containing considerably more information about the ambient traffic ...of high resolution mm-wave radar with respect ... See full document

7

84 GHz methanol masers, their relationship to 36 GHz methanol masers, and their molecular environments

84 GHz methanol masers, their relationship to 36 GHz methanol masers, and their molecular environments

... has high-resolution source maps that break the distributed maser emission into components while our spectra have blended all of the components into one single ... See full document

22

The relationship between Class I and Class II methanol masers at high angular resolution

The relationship between Class I and Class II methanol masers at high angular resolution

... from class II methanol masers, class I emission appears to be considerably sim- ...multiple class I transitions observed from the same masing region often appear as single ... See full document

18

Class I methanol masers in NGC253: alcohol at the end of the bar

Class I methanol masers in NGC253: alcohol at the end of the bar

... of methanol show significant differences in their sensitivity to the proton-to-electron mass ratio μ (Levshakov et ...Galactic methanol masers have been demonstrated to have the emission from the ... See full document

12

Methanol Masers: Reliable Tracers of the Early Stages of High mass Star Formation

Methanol Masers: Reliable Tracers of the Early Stages of High mass Star Formation

... of class II methanol masers invoke excitation to the second tor- sional state from the radiative field of warm dust at sub-millimeter and far-infrared (FIR) wavelengths to explain the ... See full document

45

VLA Survey of dense gas in extended green objects : prevalence of 25 GHz methanol masers

VLA Survey of dense gas in extended green objects : prevalence of 25 GHz methanol masers

... H II region ...higher resolution and poorer sensitivity of those data, there is no overlap in the centimeter continuum and extended ...angular resolution and sensitivity continuum observations are ... See full document

19

Disk Outflow Models as Applied to High Mass Star Forming Regions through Methanol and Water Maser Observations

Disk Outflow Models as Applied to High Mass Star Forming Regions through Methanol and Water Maser Observations

... predict methanol masers are pumped by infrared dust emission in the vicinity of high-mass ...GHz Class I and 6.7 GHz Class II methanol masers in 20 sources with the ... See full document

28

MALT 45: a 7mm survey of the southern Galaxy   II  ATCA follow up observations of 44GHz class I methanol masers

MALT 45: a 7mm survey of the southern Galaxy II ATCA follow up observations of 44GHz class I methanol masers

... tected by very-long-baseline interferometry and single-dish/auto- correlation observations. These comparisons between cross- and auto-correlation data reveal a significant amount of resolved-out flux density; Bartkiewicz ... See full document

40

High mass starless clumps in the inner galactic plane: the sample and dust properties

High mass starless clumps in the inner galactic plane: the sample and dust properties

... with Class II methanol masers and H  II  regions, suggesting that they will evolve into star-forming ...forming high- mass ...of high-mass star ...possible ... See full document

17

A comparative evaluation of position and orientation of hyoid bone in skeletal class i, class ii and class iii subjects: a cephalometric study

A comparative evaluation of position and orientation of hyoid bone in skeletal class i, class ii and class iii subjects: a cephalometric study

... comparing Class I, Class II and Class III ...in Class III than in Class II subjects in relation to cervical ...and Class III) was ...in Class I normal, ... See full document

5

Ultrasonographic evaluation of the circumoral musculature in skeletal class I and skeletal class ii division 1 malocclusion subjects: A comparative study

Ultrasonographic evaluation of the circumoral musculature in skeletal class I and skeletal class ii division 1 malocclusion subjects: A comparative study

... , 1965; HeliVinkka-Puhakka et al., this causes the lower lip to touch the palatal surface of incisors, which causes lower lip hyper function. Swallowing this way may maintain or increase the overjet, and contraction of ... See full document

5

Comparison of high-resolution Scheimpflug and high-frequency ultrasound biomicroscopy to anterior-segment OCT corneal thickness measurements

Comparison of high-resolution Scheimpflug and high-frequency ultrasound biomicroscopy to anterior-segment OCT corneal thickness measurements

... GmbH, Wetzlar, Germany), a spectral-domain AS-OCT (RTVue-100, Optovue Inc, Fremont, CA, USA), and a high- frequency ultrasound biomicroscopy (HF-UBM) system (Artemis II, Artemis Medical Technologies Inc, ... See full document

9

Dendritic diversification through transcription factor mediated suppression of alternative morphologies

Dendritic diversification through transcription factor mediated suppression of alternative morphologies

... Fig. 6. Sd and Vg are required for low Cut expression levels in ddaB. (A) Anti-HRP labeling of control dorsal cluster. Individual da neurons are named. (A ′ ) Anti-Cut labeling of dorsal cluster neurons in grayscale ... See full document

12

Bag of Features Based Remote Sensing Image Classification Using RANSAC And SVM

Bag of Features Based Remote Sensing Image Classification Using RANSAC And SVM

... SIFT keypoints are used for feature extraction. It has the following features. It has rich information and is suitable for fast and accurate features in huge data set and will produce a large number of feature vectors ... See full document

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