Zobrazeno 1 - 10
of 11
pro vyhledávání: '"Achim Tappe"'
Publikováno v:
EAS Publications Series. 46:169-175
I present observations of shock-processed PAHs and dust in supernova remnants (SNRs). Supernova shocks are one of the primary sites destroying, fragmenting and altering interstellar PAHs and dust. Studies of PAHs through supernova shocks had been lim
Autor:
Elizabeth A. Lada, Charles J. Lada, Thomas P. Robitaille, Jan Forbrich, A. Stolte, Paula S. Teixeira, Achim Tappe, August Muench
Publikováno v:
The Astrophysical Journal. 716:1453-1477
When studying the evolutionary stages of protostars that form in clusters, the role of any intracluster medium cannot be neglected. High foreground extinction can lead to situations where young stellar objects (YSOs) appear to be in earlier evolution
Autor:
Una Hwang, William T. Reach, Jonathan D. Slavin, Takashi Kozasa, Achim Tappe, Jeonghee Rho, Loretta Dunne
Publikováno v:
The Astrophysical Journal. 700:579-596
We present Spitzer Infrared Spectrograph and Infrared Array Camera observations of the young supernova remnant E0102 (SNR 1E0102-7219) in the Small Magellanic Cloud. The infrared spectra show strong lines of Ne and O, with the [Ne II] line at 12.8 μ
Autor:
Dohy Faied, Jeonghee Rho, Francesco Palla, Patrick W. Morris, R. Valdettaro, Thomas H. Jarrett, L. Cambrésy, William T. Reach, Adwin Boogert, Achim Tappe
Publikováno v:
The Astrophysical Journal. 690:683-705
Extremely red objects, identified in the early Spitzer Space Telescope observations of the bright-rimmed globule IC 1396A and photometrically classified as Class I protostars Class II T Tauri stars based on their mid-infrared colors, were observed sp
Autor:
Achim Tappe, John H. Black
Publikováno v:
Astronomy & Astrophysics. 423:943-954
We report Very Large Telescope (VLT) observations of the quasar PKS 2145+067. We obtained high-resolution (R ≈ 100 000 or 3 km s −1 ) optical spectra with the UV-Visual Echelle Spectrograph (UVES) at the VLT UT2 telescope. The emission redshift m
Autor:
Knox S. Long, P. Frank Winkler, Sangwook Park, Parviz Ghavamian, John C. Raymond, William P. Blair, Achim Tappe
We present mid-infrared (5-40 micron) spectra of shocked ejecta in the Galactic oxygen-rich supernova remnant G292.0+1.8, acquired with the IRS spectrograph on board the Spitzer Space Telescope. The observations targeted two positions within the brig
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::786dbe8f83d82b70a630a139fa239cad
We present a 5-37 micron infrared spectrum obtained with the Spitzer Space Telescope toward the southeastern lobe of the young protostellar outflow HH211. The spectrum shows an extraordinary sequence of OH emission lines arising in highly excited rot
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2f4ca63dd98e2e8358e2ee9c4a546262
We observed the oxygen-rich Large Magellanic Cloud (LMC) supernova remnant N132D (SNR 0525-69.6), using all instruments onboard the Spitzer Space Telescope, IRS, IRAC, and MIPS (Infrared Spectrograph, Infrared Array Camera, Multiband Imaging Photomet
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8990af24f9dbd032db805865e17dc7ed
https://resolver.caltech.edu/CaltechAUTHORS:20110629-113443726
https://resolver.caltech.edu/CaltechAUTHORS:20110629-113443726
Autor:
Thomas G. Pannuti, Marilyn R. Meade, Ed Churchwell, William T. Reach, Crystal L. Brogan, Jeonghee Rho, Achim Tappe, Remy Indebetouw, Brian Babler, Barbara A. Whitney
Using Infrared Array Camera (IRAC) images at 3.6, 4.5, 5.8, and 8 microns from the GLIMPSE Legacy science program on the Spitzer Space Telescope, we searched for infrared counterparts to the 95 known supernova remnants that are located within galacti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ccfc0b40023273a8acfac75516e7b9d0
Publikováno v:
The Astrophysical Journal. 754:132
We present Spitzer Infrared Spectrograph 14-36 ?m mapping observations of the supernova remnant N132D in the Large Magellanic Cloud. This study focuses on the processing of polycyclic aromatic hydrocarbons (PAHs) that we previously identified in the