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1921. http://www.mso.anu.edu.au/seminars/abstracts/20151215-1100.html
Following the East Asian Observatory assuming operations of the James Clerk Maxwell Observatory in March 2015, the Observatory has had an extremely successful and productive year. ... The EAO intends to accelerate these achievements by embarking on an ambitious program of instrument upgrades and additions that will further extend the JCMT s capabilities. An overview of the East Asian Observatory and its vision will be described, and the JCMT operations and capabilities will be presented. ...
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151215-1100.html -- 4.6 Кб -- 10.04.2016
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1922. http://www.mso.anu.edu.au/seminars/abstracts/20151211-1400.html
I review some of what IтАЩve recently learned about the portrayal by and of women in Hollywood productions. I first discuss how women are under-represented in roles as writers, directors, cinematographers, etc, some of the discussion around the issue, and in contrast how many men manage to make it to the top of the queue fairly quickly. ...
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151211-1400.html -- 4.2 Кб -- 10.04.2016
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1923. http://www.mso.anu.edu.au/seminars/abstracts/20151210-1100.html
The most fundamental unsolved problems in galaxy formation revolve around "feedback" from massive stars and black holes. I ll present new simulations which combine new numerical methods and physics in an attempt to realistically model the diverse physics of the interstellar medium, star formation, and feedback from stellar radiation pressure, supernovae, stellar winds, and photo-ionization. ...
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151210-1100.html -- 5.3 Кб -- 10.04.2016
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1924. http://www.mso.anu.edu.au/seminars/abstracts/20151209-1100.html
Recent molecular observations indicate supersonic cloud-cloud collision is one of the important modes of O star formation. The O star formation regions studied so far include super star clusters (Westerlund2, NGC3603, RCW38 etc.), mini-starbursts (NGC6334, NGC6357 etc.) HII regions (M42/43, M20 etc.), and Spitzer bubbles (RCW120 etc.) ... Since the collision time scale is short ~10^5 yrs, O star formation is a rapid process with a mass accretion rate higher than 10^-4Mo/yr. ...
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151209-1100.html -- 4.3 Кб -- 10.04.2016
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1925. http://www.mso.anu.edu.au/seminars/abstracts/20151204-0900.html
. A number of student talks will be presented.
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151204-0900.html -- 3.7 Кб -- 10.04.2016
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1926. http://www.mso.anu.edu.au/seminars/abstracts/20151203-0900.html
. A number of student talks will be presented.
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151203-0900.html -- 3.7 Кб -- 10.04.2016
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1927. http://www.mso.anu.edu.au/seminars/abstracts/20151201-1100.html
... In this talk I present a summary of my PhD thesis, which investigates the characteristics, formation and dynamics of filaments arising from wind-cloud interactions. I use magnetohydrodynamic numerical simulations with gas multi-tracking techniques to shed light on the physical mechanisms acting upon wind-swept clouds and provide measurements of the aspect ratios, internal velocity dispersions, energy densities, and magnetic field strengths and orientations in the resulting filaments. ...
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151201-1100.html -- 4.8 Кб -- 10.04.2016
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1928. http://www.mso.anu.edu.au/seminars/abstracts/20151127-1400.html
. The Zooniverse has created an online interface, Panoplies, where you can develop your own visualisation portal that can be made public or private. In this talk I will discuss some of the ways you can utilise this online system for your own research even if you know nothing about web design.
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151127-1400.html -- 4.0 Кб -- 10.04.2016
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1929. http://www.mso.anu.edu.au/seminars/abstracts/20151126-1100.html
In 2011 the Nobel Prize in Physics was awarded "for the discovery of the accelerating expansion of the Universe through observations of distant supernovae". These Type Ia supernovae (SNe Ia) are also the dominant contributor to iron-group nucleosynthesis and leading candidates for the elusive sites of high energy cosmic rays, the p-process isotopes, and the positrons responsible for the 511 keV annihilation signal in our Galaxy. ...
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151126-1100.html -- 4.9 Кб -- 10.04.2016
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1930. http://www.mso.anu.edu.au/seminars/abstracts/20151124-1100.html
We present spectral line images of [CI] 809 GHz, CO J=1-0 110 115 GHz and HI 1.4 GHz line emission along a ~1ТА region in the l=328ТА direction of the Galactic plane. The [CI] data comes from the High Elevation Antarctic Terahertz (HEAT) telescope, a new facility on the summit of the Antarctic plateau where the precipitable water vapour falls to the lowest values found on the surface of the Earth. ... The [C/CO] abundance ratio averaged through the filament is found to be approximately unity. ...
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151124-1100.html -- 5.7 Кб -- 10.04.2016
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1931. http://www.mso.anu.edu.au/seminars/abstracts/20151120-1420.html
. I will introduce the work I will be doing for my Masters Thesis. I will first give background on protoplanetary disks and their structures and features and then discuss which disks I will be studying and give an overview of the methods I will use to do this.
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151120-1420.html -- 4.0 Кб -- 10.04.2016
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1932. http://www.mso.anu.edu.au/seminars/abstracts/20151120-1400.html
For around forty years, astrophysicists have observed the annihilation of positrons in the Galaxy at a prodigious rate. ... The fact the Galactic bulge far outshines the disk in annihilating positrons which are injected into the ISM at low energies makes the source of the positrons difficult to identify, as the main source of such positrons are prima facie located in the Galactic disk. ...
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151120-1400.html -- 4.8 Кб -- 10.04.2016
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1933. http://www.mso.anu.edu.au/seminars/abstracts/20151119-1100.html
... By taking advantage of atomic hydrogen (HI) observations obtained as part of the GALEX Arecibo SDSS and ALFALFA surveys, I will demonstrate that the combination of deep, targeted observations and spectral stacking of blind, large-area shallow surveys is critical in order to characterize how the gas content of galaxies depends on their structure, star formation activity and environment. ...
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151119-1100.html -- 4.9 Кб -- 10.04.2016
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1934. http://www.mso.anu.edu.au/seminars/abstracts/20151113-1400.html
. TBD .
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151113-1400.html -- 3.8 Кб -- 10.04.2016
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1935. http://www.mso.anu.edu.au/seminars/abstracts/20151112-1100.html
... Their large amounts of dust make them ideal objects to study how dust forms in the high-redshift interstellar medium (ISM), and to study the interplay between star formation activity, gas and dust. Up until recent interferometric observations with PdBI and ALMA, the full characterisation of SMGs had been hindered by the large beams of single-dish observations that made it challenging to identify their optical and infrared counterparts. ...
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151112-1100.html -- 5.7 Кб -- 10.04.2016
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1936. http://www.mso.anu.edu.au/seminars/abstracts/20151110-1100.html
Data from the VVV NIR survey of the inner Milky Way show that our Galaxy has a strongly peanut-shaped bulge. Extending the analysis to larger radii with other surveys shows that the long bar is aligned with the bulge and extends to about 30 degrees longitude. ... The Milky Way bulge appears to have been mostly formed from the disk through a bar and buckling instability, with little evidence for a classical , merger-built bulge. ...
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151110-1100.html -- 4.5 Кб -- 10.04.2016
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1937. http://www.mso.anu.edu.au/seminars/abstracts/20151106-1420.html
I will present theresults from a deep, extended, planetary nebulae survey in a 0.5 sqdeg region centered on the brightest cluster galaxy NGC 4486 (M87) in the Virgo cluster core, carried out with SuprimeCam@Subaru and FLAMES-GIRAFFE@VLT. ... A substructure detected in the projected phase-space of the line-of-sight velocity vs. major axis distance for the M87 halo planetary nebulae provides evidence for the recent accretion event of a satellite galaxy with luminosity twice that of M33. ...
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151106-1420.html -- 5.0 Кб -- 10.04.2016
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1938. http://www.mso.anu.edu.au/seminars/abstracts/20151106-1400.html
. 10 Gyr old ~solar mass stars which have only recently run through their main sequence lifetimes. In our scenario, then, the positrons are echoes of the last big burst of bulge star-formation at z ~ 2. Similar WD-WD collisions, occurring in the thick disk, ultimately supply much of the 511 keV radiation emission extending along the Galactic plane.
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151106-1400.html -- 4.7 Кб -- 10.04.2016
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1939. http://www.mso.anu.edu.au/seminars/abstracts/20151029-1100.html
Aboriginal and Torres Strait Islander people developed complex knowledge systems around the sun, moon, and stars. Stellar positions and properties (such as declination, colour, brightness, and scintillation) were important for navigation, calendars, economics, and time-keeping. Transient astronomical phenomena (including comets, meteors, eclipses, and aurorae) reinforced sacred law and cultural practices and served as a moral charter. ...
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151029-1100.html -- 4.4 Кб -- 10.04.2016
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1940. http://www.mso.anu.edu.au/seminars/abstracts/20151027-1100.html
The spectra of AGN host galaxies contain emission lines excited by radiation from both massive stars and the AGN accretion disk. ... I will present the first 2D maps of the star formation rates across AGN host galaxies without contamination from the AGN, and the first maps of the narrow line region emission without contamination from star formation. ...
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151027-1100.html -- 4.8 Кб -- 10.04.2016
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