2015年8月31日月曜日

Galactic Rotation Curves with Dark Matter Self-Interactions

Dr. Ayuki Kamada (UC Riverside)
2015-08-31 
ISAS seminar

Abstract: 
It has been shown that the LambdaCDM model can successfully explain large-scale structure of the universe. But it is not clear that it can accommodate observations on (sub-)galactic scales. In fact, the LambdaCDM model predicts dark matter halos, which are systematically denser than inferred from astrophysical observations. One interesting alternative assumes that dark matter particles are strongly interacting with each other. Dark matter self-interactions will lead to heat transfer from the hotter outer region to the cold inner region, reducing the central dark matter density. In this talk, I will show that the observed rotation curves of spiral galaxies are consistent with predicted in the SIDM model. I will also emphasize the importance of the baryonic disk in determining the SIDM halo profile.

2015年8月27日木曜日

looking into X-ray spectra

I have been looking into these kinds of X-ray spectra from the hot universe.
For some long time…
Can I discover something new from these data further more ?
Or need brand new instruments ?

2015年8月18日火曜日

Life, the multiverse and everything

economist, 2015-08-08
http://www.economist.com/news/leaders/21660537-science-has-remade-world-scientists-are-not-finished-yet-life-multiverse-and


The Exploration of Pluto and the Kuiper Belt with the New Horizons Mission

Space Science Seminar

Speaker: Dr. Harold (Hal) Weaver
(The Johns Hopkins University Applied Physics Laboratory)

Title:
The Exploration of Pluto and the Kuiper Belt with the New Horizons Mission

Abstract:
The New Horizons (NH) mission was selected by NASA in November 2001 to
conduct the first in situ reconnaissance of Pluto and the Kuiper belt.
The NH spacecraft was launched on 2006 January 19, received a gravity 
assist from Jupiter during closest approach on 2007 February 28, and
flew 12,500 km above Pluto's surface on 2015 July 14. NH carries a
sophisticated suite of seven scientific instruments, altogether weighing
less than 30 kg and drawing less than 30 W of power, that includes
panchromatic and color imagers, ultraviolet and infrared spectral
imagers, a radio science package, plasma and charged particle sensors,
and a dust counting experiment. These instruments enabled the first
detailed exploration of a new class of solar system objects, the dwarf
planets, which have exotic volatiles on their surfaces, escaping
atmospheres, and satellite systems. NH also provided the first dust
density measurements beyond 18~AU and cratering records that document
both the ancient and present-day collisional environment in the outer
solar system down to sizes of tens of meters. NH obtained unprecedented
data on Pluto’s small satellites (Styx, Nix, Kerberos, and Hydra),
adding significantly to the scientific bounty returned from the NH
mission. The NH spacecraft will be targeted toward the flyby of a small
(~30 km) KBO in late-2015, enabling the study of an object in a
completely different dynamical class (cold classical) than Pluto, if
NASA approves an Extended Mission phase.

http://pluto.jhuapl.edu




2015年8月6日木曜日

Luminous Supermassive Black Holes in the Brightest Cluster Galaxies

2015-08-06 ISAS astro seminar

Shutaro Ueda (ISAS/JAXA)

Title: 
Abstract:
Supermassive black holes (SMBHs) in the central galaxies of clusters of galaxies (i.e.,
in the brightest cluster galaxies; BCGs) are the most massive BH in the Universe. Their
masses are estimated to be up to 1011 M. The SMBHs in nearby BCGs have a slight gas
accretion rate, which is typically less than 1 % of the Eddington limit. This indicates
that their mass growth may be performed at the early stage of evolution of their hosted
cluster. However its mechanism is still under debate. We therefore search for quasar
hosted BCGs (i.e., with high accretion rate) systematically by referring both the Planck
SZ cluster catalogue and the Swift hard X-ray catalogue. We find two sources out of 1203
clusters, which are the Phoenix cluster and H1821+643 cluster. We also investigate their
surrounding environment by using X-ray observations with Chandra and Suzaku. We find the
neutral iron K-shell line (Fe I) from both quasars and heavily absorption component from
the quasar of the Phoenix cluster. We discuss the environments of both quasars and the
origin of neutral medium surrounding quasars.