Zobrazeno 1 - 10
of 25 485
pro vyhledávání: '"AKARI"'
Autor:
Clayton Barreto
CLAYTON BARRETO estreia no mundo editorial com Akari – uma ilusão nipônica, conto premiado com menção honrosa pela Fundação Cultural Capitania das Artes. Nesta obra narra de forma ficcional a busca de uma jovem pelo pai perdido no Japão, os
Autor:
Kim, Helen Kyung, Malkan, Matthew A., Takagi, Toshinobu, Oi, Nagisa, Burgarella, Denis, Miyaji, Takamitsu, Shim, Hyunjin, Matsuhara, Hideo, Goto, Tomotsugu, Ohyama, Yoichi, Buat, Veronique, Kim, Seong Jin
Polycyclic aromatic hydrocarbon (PAH) dust emission has been proposed as an effective extinction-independent star formation rate (SFR) indicator in the mid-infrared (MIR), but this may depend on conditions in the interstellar medium. The coverage of
Externí odkaz:
http://arxiv.org/abs/2408.14005
Autor:
Kondo, Tsubasa, Kondo, Akino, Murata, Katsuhiro L., Kokusho, Takuma, Oyabu, Shinki, Suzuki, Toyoaki, Katayama, Risako, Kaneda, Hidehiro
Hydrocarbon dust is one of the dominant components of interstellar dust, which mainly consists of polycyclic aromatic hydrocarbons and aliphatic hydrocarbons. While hydrocarbon dust is thought to be processed in interstellar radiation fields or shock
Externí odkaz:
http://arxiv.org/abs/2407.13454
Identification of planetary and proto-planetary nebulae candidates through akari infrared photometry
Autor:
Marquez-Lugo, R. A., Kemp, S. N., Ramos-Larios, G., Nigoche-Netro, A., Navarro, S. G., Corral, L. J.
Publikováno v:
RMxAA. Vol. 60, N{\deg}2, October 2024
We utilized photometric data from the space telescope AKARI to identify potential planetary nebulae (PNe) and proto-planetary nebulae (PPNe) candidates. Using the colour-colour diagram, we found a region with a high concentration of established PNe a
Externí odkaz:
http://arxiv.org/abs/2407.16060
Autor:
Miyaji, T., Bravo-Navarro, B. A., Tello, J. Díaz, Krumpe, M., Herrera-Endoqui, M., Ikeda, H., Takagi, T., Oi, N., Shogaki, A., Matsuura, S., Kim, H., Malkan, M. A., Hwang, H. S., Kim, T., Ishigaki, T., Hanami, H., Kim, S. J., Ohyama, Y., Goto, T., Matsuhara, H.
Publikováno v:
A&A 689, A83 (2024)
We present a catalog of optical and infrared identifications (ID) of X-ray sources in the AKARI North Ecliptic Pole (NEP) Deep field detected with Chandra covering $\sim 0.34\,{\rm deg^{2}}$ with 0.5-2 keV flux limits ranging $\sim 2 \mathrm{-} 20\ti
Externí odkaz:
http://arxiv.org/abs/2407.13864
Akademický článek
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Publikováno v:
Bibechana, Vol 21, Iss 1 (2024)
This work presents the comparative study of the properties of dust within the W51 Giant Molecular Cloud (GMC) located at (RA, DEC) (J2000): 290.91°, +14.51°. In the infrared data of Improved Reprocessing of the IRAS (IRIS) the dust structure seems
Externí odkaz:
https://doaj.org/article/430ebbd701874d53b0768b77c0005384
Publikováno v:
The Astrophysical Journal, Volume 944, Number 2, article id.202 (2023)
(704) Interamnia is one of the largest asteroids that locates in the outer main-belt region, which may contain a large amount of water ice underneath its surface. We observe this asteroid using 8.2 m Subaru telescope at mid-infrared wavebands, and ut
Externí odkaz:
http://arxiv.org/abs/2212.09534
Autor:
Shim, Hyunjin, Hwang, Ho Seong, Jeong, Woong-Seob, Toba, Yoshiki, Kim, Minjin, Kim, Dohyeong, Song, Hyunmi, Hashimoto, Tetsuya, Nakagawa, Takao, Nanni, Ambra, Pearson, William J., Takagi, Toshinobu
We investigate the variation in the mid-infrared spectral energy distributions of 373 low-redshift ($z<0.4$) star-forming galaxies, which reflects a variety of polycyclic aromatic hydrocarbon (PAH) emission features. The relative strength of PAH emis
Externí odkaz:
http://arxiv.org/abs/2212.04635
Autor:
Kim, Jaeyeong, Lee, Jeong-Eun, Jeong, Woong-Seob, Kim, Il-Seok, Aikawa, Yuri, Noble, Jeniffer A., Choi, Minho, Lee, Ho-Gyu, Dunham, Michael M., Kim, Chul-Hwan, Koo, Bon-Chul
We present near-infrared spectra of three low-luminosity protostars and one background star in the Perseus molecular cloud, acquired using the Infrared Camera (IRC) onboard the \textit{AKARI} space telescope. For the comparison with different star-fo
Externí odkaz:
http://arxiv.org/abs/2207.05178