output
19972026
most citedThe Infrared Astronomical Mission AKARI

842 citations

Showing 2009Show all

7 papers · 1 filter

astro-ph.GA2009★ 11 cited

Properties of active galactic star-forming regions probed by imaging spectroscopy with the Fourier transform spectrometer (FTS) onboard AKARI

Yoko Okada, Mitsunobu Kawada, Noriko Murakami +8

We investigate the structure of the interstellar medium (ISM) and identify the location of possible embedded excitation sources from far-infrared (FIR) line and mid-infrared contin…

astro-ph.HE2009★ 165 cited

Early phase observations of extremely luminous Type Ia Supernova 2009dc

M. Yamanaka, K. S. Kawabata, K. Kinugasa +31

We present early phase observations in optical and near-infrared wavelengths for the extremely luminous Type Ia supernova (SN Ia) 2009dc. The decline rate of the light curve is $Δm…

astro-ph.SR2009★ 81 cited

BD +44 493: A Ninth Magnitude Messenger from the Early Universe; Carbon Enhanced and Beryllium Poor

Hiroko Ito, Wako Aoki, Satoshi Honda +1

We present a 1D LTE chemical abundance analysis of the very bright (V=9.1) Carbon-Enhanced Metal-Poor (CEMP) star BD +44 493, based on high-resolution, high signal-to-noise spectra…

astro-ph.SR2009★ 18 cited

Spectroscopic Observations of the WZ Sge-Type Dwarf Nova GW Librae during the 2007 Superoutburst

Kazuo Hiroi, Daisaku Nogami, Yoshihiro Ueda +13

We carried out an international spectroscopic observation campaign of the dwarf nova GW Librae (GW Lib) during the 2007 superoutburst. Our observation period covered the rising pha…

astro-ph.HE2009★ 28 cited

Early Spectral Evolution of the Rapidly Expanding Type Ia SN 2006X

Masayuki Yamanaka, Hiroyuki Naito, Kenzo Kinugasa +6

We present optical spectroscopic and photometric observations of Type Ia supernova (SN) 2006X from --10 to +91 days after the -band maximum. This SN exhibits one of the highest…

astro-ph.HE2009★ 19 cited

Doppler-Broadened Iron X-ray Lines from Tycho's Supernova Remnant

A. Furuzawa, D. Ueno, A. Hayato +13

We use \suzaku observations to measure the spatial variation of the Fe K line with radius in the \tycho supernova remnant. The Fe line widths show a significant decrease from a…