VIEW CV - EMDL - University of Delhi
... “Dielectric dispersion of rf sputtered deposited SnO2, ZnO, WO3 thin films using Surface Plasmon Resonance Technique”. Ayushi Paliwal, Anjali Sharma, Monika Tomar and Vinay Gupta, IEEE Tranactions on Dielectrics and Electrical Insulation, (2015) in press. “A highly efficient urea detection using flo ...
... “Dielectric dispersion of rf sputtered deposited SnO2, ZnO, WO3 thin films using Surface Plasmon Resonance Technique”. Ayushi Paliwal, Anjali Sharma, Monika Tomar and Vinay Gupta, IEEE Tranactions on Dielectrics and Electrical Insulation, (2015) in press. “A highly efficient urea detection using flo ...
Galaxy Formation and Evolution.
... S I M O N W H I T E is Director at the Max Planck Institute for Astrophysics in Garching. He is one of the originators of the modern theory of galaxy formation and has received numerous international prizes and honors. ...
... S I M O N W H I T E is Director at the Max Planck Institute for Astrophysics in Garching. He is one of the originators of the modern theory of galaxy formation and has received numerous international prizes and honors. ...
Physics of Neutron Star Crusts - Institut d`Astronomie et d
... of comparison, we describe also another EoS of matter at subnuclear density – that relevant for the collapsing type II supernova core. Section 6 is devoted to the stellar structure aspects of neutron star crust. We start with the simplest case of a spherically symmetric static neutron star and deriv ...
... of comparison, we describe also another EoS of matter at subnuclear density – that relevant for the collapsing type II supernova core. Section 6 is devoted to the stellar structure aspects of neutron star crust. We start with the simplest case of a spherically symmetric static neutron star and deriv ...
Physics of Neutron Star Crusts
... of comparison, we also describe another EoS of matter at subnuclear density – that relevant for the collapsing type II supernova core. Section 6 is devoted to the stellar-structure aspects of neutron star crusts. We start with the simplest case of a spherically-symmetric static neutron star and deri ...
... of comparison, we also describe another EoS of matter at subnuclear density – that relevant for the collapsing type II supernova core. Section 6 is devoted to the stellar-structure aspects of neutron star crusts. We start with the simplest case of a spherically-symmetric static neutron star and deri ...
CONSTRUCTING A PYTHON PIPELINE FOR ANALYZING
... Possible line blending of crowded molecular emission lines was an important obstacle in determining the frequency/velocity range defined to encompass each emission line. While we assume a constant velocity dispersion across the entire source, performing more rigorous LTE modeling in various regions ...
... Possible line blending of crowded molecular emission lines was an important obstacle in determining the frequency/velocity range defined to encompass each emission line. While we assume a constant velocity dispersion across the entire source, performing more rigorous LTE modeling in various regions ...
![[CII] in the nuclear region of M33: HerM33es](http://s1.studyres.com/store/data/016974860_1-2848b26c9bc0383003a9db0691112ce5-300x300.png)
ASTE Simultaneous HCN(4–3) and HCO+(4–3)
... and HCO+ observations in both data make the discussion of HCN to HCO+ flux ratios reliable, and (2) HCN(1–0) and HCO+ (1–0) absolute fluxes in the NMA data are confirmed to agree with other single dish telescope’s measurements (Imanishi et al. 2004, 2007b). NMA measurements of HCN(1–0) and HCO+ (1–0 ...
... and HCO+ observations in both data make the discussion of HCN to HCO+ flux ratios reliable, and (2) HCN(1–0) and HCO+ (1–0) absolute fluxes in the NMA data are confirmed to agree with other single dish telescope’s measurements (Imanishi et al. 2004, 2007b). NMA measurements of HCN(1–0) and HCO+ (1–0 ...
The Twenty-fourth Colloquium on High Resolution Molecular
... to mark the HRMS 2015 conference. All participants of the conference are invited to contribute a paper. This is not intended to be a conference proceedings, but rather a collection of original research papers, related to the conference themes and to material presented at the conference either as tal ...
... to mark the HRMS 2015 conference. All participants of the conference are invited to contribute a paper. This is not intended to be a conference proceedings, but rather a collection of original research papers, related to the conference themes and to material presented at the conference either as tal ...
Formation and evolution of giant molecular clouds in a barred spiral
... surface densities follow a nearly linear trend in all three galactic environments. There is a small deviation towards a steeper gradient at densities below ∼10 M⊙ pc−2 and also an increased scatter due to the smaller number of clouds found within our measured region. Note that this change has a diff ...
... surface densities follow a nearly linear trend in all three galactic environments. There is a small deviation towards a steeper gradient at densities below ∼10 M⊙ pc−2 and also an increased scatter due to the smaller number of clouds found within our measured region. Note that this change has a diff ...
Giant Low Surface Brightness Galaxies
... in our Universe. Hα observations of the larger LSB disk galaxies and especially GLSB galaxies reveal that they have patches of localized star formation (e.g. Auld et al. 2006) associated with faint spiral arms or distributed sporadically over their disks. Surprisingly, in spite of their low Star For ...
... in our Universe. Hα observations of the larger LSB disk galaxies and especially GLSB galaxies reveal that they have patches of localized star formation (e.g. Auld et al. 2006) associated with faint spiral arms or distributed sporadically over their disks. Surprisingly, in spite of their low Star For ...
First Results from the WISE Enhanced Resolution Galaxy Atlas
... dow of the electromagnetic spectrum, from the radio to the X-ray, provides a complementary set of tools that, in combination, reveal the internal life cycle of galaxies. The infrared window, for example, has dual capability: sensitive to stellar light from the evolved population of stars and relativ ...
... dow of the electromagnetic spectrum, from the radio to the X-ray, provides a complementary set of tools that, in combination, reveal the internal life cycle of galaxies. The infrared window, for example, has dual capability: sensitive to stellar light from the evolved population of stars and relativ ...
![arXiv:1601.01542v1 [astro-ph.GA] 7 Jan 2016](http://s1.studyres.com/store/data/017487687_1-243c4cbda96da53325dd347b0c588a3e-300x300.png)
arXiv:1601.01542v1 [astro-ph.GA] 7 Jan 2016
... redshift on the stellar mass-size relation. According to the insideout growth of discs, galaxies are expected to increase their scale lengths with time as they grow in mass (Barden et al. 2005; Trujillo et al. 2004, 2006), resulting in a constant mass-size relation with cosmic time. In this context, ...
... redshift on the stellar mass-size relation. According to the insideout growth of discs, galaxies are expected to increase their scale lengths with time as they grow in mass (Barden et al. 2005; Trujillo et al. 2004, 2006), resulting in a constant mass-size relation with cosmic time. In this context, ...
Gas Evolution in Disk Galaxies
... ’SBa’. These galaxies are also the most tightly wound spirals. Those with the least bulge-todisk luminosity ratios and the most open spirals are classified as ‘Sc’ or ’SBc’. Whereas, the intermediate ones are classified as ’Sb’ or ’SBb’. Lenticulars are disk galaxies without visible spirals. Due to ...
... ’SBa’. These galaxies are also the most tightly wound spirals. Those with the least bulge-todisk luminosity ratios and the most open spirals are classified as ‘Sc’ or ’SBc’. Whereas, the intermediate ones are classified as ’Sb’ or ’SBb’. Lenticulars are disk galaxies without visible spirals. Due to ...
2010 Middle School Science - Summer School Pacing Guide
... Objective: 1) TSW recall the definition of a chemical element. 2) TSW identify elements by their chemical symbols. 8-2d Describe cause and effect relationships of electrical energy –Relate how electrical energy transfers through electric circuits (using common pictures and symbols) ...
... Objective: 1) TSW recall the definition of a chemical element. 2) TSW identify elements by their chemical symbols. 8-2d Describe cause and effect relationships of electrical energy –Relate how electrical energy transfers through electric circuits (using common pictures and symbols) ...
PDF file
... the stored huge energy is released into the solar atmosphere in a short time. As a result of the energy release, a lot of phenomena are observed in various wavelengths; ejections of plasma, post-flare loops, nonthermal emission from energetic particles, and so on. Magnetic reconnection is widely acc ...
... the stored huge energy is released into the solar atmosphere in a short time. As a result of the energy release, a lot of phenomena are observed in various wavelengths; ejections of plasma, post-flare loops, nonthermal emission from energetic particles, and so on. Magnetic reconnection is widely acc ...
Giant Molecular Clouds in Local Group Galaxies
... is a good value to use in most galaxies (except the SMC) if the GMCs are virialized. However, if the clouds are only marginally self-gravitating, as appears to be the case judging from their appearance, half the virial value may be more appropriate. There is no clear trend of XCO with metallicity. T ...
... is a good value to use in most galaxies (except the SMC) if the GMCs are virialized. However, if the clouds are only marginally self-gravitating, as appears to be the case judging from their appearance, half the virial value may be more appropriate. There is no clear trend of XCO with metallicity. T ...
Jets and Outflows From Star to Cloud: Observations Confront Theory
... also affect disk evolution and planet formation through disk irradiation or shielding, and enhanced radial mixing of both gas and solids. In this chapter we address this central question of outflow feedback on star and planet formation while also reviewing the current state of jet/outflow science. F ...
... also affect disk evolution and planet formation through disk irradiation or shielding, and enhanced radial mixing of both gas and solids. In this chapter we address this central question of outflow feedback on star and planet formation while also reviewing the current state of jet/outflow science. F ...
Homi Bhabha
... by Dirac who was at Cambridge during the same period. It was also here, at the Cavendish Laboratory, that Rutherford was leading a team of scientists who were making path breaking and fundamental discoveries. He completed his Ph.D. in 1935 under the guidance of Fowler, who was also the thesis adviso ...
... by Dirac who was at Cambridge during the same period. It was also here, at the Cavendish Laboratory, that Rutherford was leading a team of scientists who were making path breaking and fundamental discoveries. He completed his Ph.D. in 1935 under the guidance of Fowler, who was also the thesis adviso ...
Microplasma
Microplasmas are plasmas of small dimensions, ranging from tens to thousands of micrometers. They can be generated at a variety of temperatures and pressures, existing as either thermal or non-thermal plasmas. Non-thermal microplasmas that can maintain their state at standard temperatures and pressures are readily available and accessible to scientists as they can be easily sustained and manipulated under standard conditions. Therefore, they can be employed for commercial, industrial, and medical applications, giving rise to the evolving field of microplasmas.