Zobrazeno 1 - 10
of 19
pro vyhledávání: '"Jeonghee Rho"'
Autor:
Jeniveve Pearson, Griffin Hosseinzadeh, David J. Sand, Jennifer E. Andrews, Jacob E. Jencson, Yize Dong, K. Azalee Bostroem, S. Valenti, Daryl Janzen, Nicolás Meza Retamal, M. J. Lundquist, Samuel Wyatt, R. C. Amaro, Jamison Burke, D. Andrew Howell, Curtis McCully, Daichi Hiramatsu, Saurabh W. Jha, Nathan Smith, Joshua Haislip, Vladimir Kouprianov, Daniel E. Reichart, Yi Yang, Jeonghee Rho
We present photometric and spectroscopic data of SN 2018lab, a low-luminosity Type IIP supernova (LLSN) with a V-band peak luminosity of −15.1 ± 0.1 mag. SN 2018lab was discovered by the Distance Less Than 40 Mpc (DLT40) SN survey only 0.73 days p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e2c18196a5512b75a1b2b14cfa7dd242
We present far-infrared (FIR) spectroscopy of supernova remnants (SNRs) based on the archival data of the Infrared Space Observatory ($ISO$) taken with the Long Wavelength Spectrometer (LWS). Our sample includes previously unpublished profiles of lin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a2f2bd55885db128ef36070aa103ba80
Autor:
H. G. Lee, Le Ngoc Tram, William T. Reach, Barbara A. Whitney, John H. Bieging, Thomas H. Jarrett, Bon-Chul Koo, Wanggi Lim, Jeonghee Rho
We present the detections of shocked molecular hydrogen (H2) gas in near- and mid-infrared and broad CO in millimeter from the mixed-morphology supernova remnant (SNR) HB~3 (G132.7+1.3) using Palomar WIRC, the Spitzer GLIMPSE360 and WISE surveys, and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::54759d7a6051a9e62d558c2536f20162
Autor:
Hamza Ajeddig, Philippe André, Pak Shing Li, Christopher F. McKee, Jeonghee Rho, Enrique Lopez-Rodriguez, Richard I. Klein
Optical and infrared polarization mapping and recent Planck observations of the filamentary cloud L1495 in Taurus show that the large-scale magnetic field is approximately perpendicular to the long axis of the cloud. We use the HAWC+ polarimeter on S
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c2c44d24570b17000cedf55d48a55c70
Publikováno v:
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2018, 864 (1), pp.L20. ⟨10.3847/2041-8213/aad77f⟩
The Astrophysical journal letters, 2018, 864 (1), pp.L20. ⟨10.3847/2041-8213/aad77f⟩
The Astrophysical journal letters, Bristol : IOP Publishing, 2018, 864 (1), pp.L20. ⟨10.3847/2041-8213/aad77f⟩
The Astrophysical journal letters, 2018, 864 (1), pp.L20. ⟨10.3847/2041-8213/aad77f⟩
The origin of dust in the early Universe has been the subject of considerable debate. Core-collapse supernovae (ccSNe), which occur several million years after their massive progenitors form, could be a major source of that dust, as in the local univ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0ec79eed70b3eef850622844ccff3522
Autor:
Haley Louise Gomez, Alberto Noriega-Crespo, Phil Cigan, Jeonghee Rho, M. J. Barlow, Loretta Dunne, Mikako Matsuura, I. De Looze, H. Chawner, Kenneth A. Marsh
Publikováno v:
Monthly Notices of the Royal Astronomical Society
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
We search for far-infrared (FIR) counterparts of known supernova remnants (SNRs) in the Galactic plane (10 deg
Comment: 33 pages and 39 figures. Accepted in MNRAS. Appendix figures are available here: https://github.com/hanchawn/Arxiv (includes
Comment: 33 pages and 39 figures. Accepted in MNRAS. Appendix figures are available here: https://github.com/hanchawn/Arxiv (includes
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d5b6f48388dd587d82c65f4293db5c55
Autor:
N. M. Ashok, Raja Rammohun Roy, Vishal Joshi, Jason Spyromilio, A. Evans, Robert D. Gehrz, Jeonghee Rho, Debabrata Banerjee, M. S. Connelley, Thomas R. Geballe, Mudit K. Srivastava
We present near-infrared spectroscopy of the NGC 5128 supernova SN 2016adj in the first 2 months following discovery. We report the detection of first overtone carbon monoxide emission at $\sim58.2$ d after discovery, one of the earliest detections o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::442f85fa0419434702a03ddcac35c104
Autor:
Oleg Kargaltsev, Jonathan W. Keohane, Jeonghee Rho, Blagoy Rangelov, Alekzander R. Kosakowski, Thomas G. Pannuti, Sonny Ernst, P. Frank Winkler, Jeremy Hare
We present a joint analysis of optical emission-line and X-ray observations of the archetypical Galactic mixed-morphology supernova remnant (MMSNR) W28 (G6.4-0.1). MMSNRs comprise a class of sources whose shell-like radio morphology contrasts with a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2c4b4cbde3ef38323d112bdf3e581d55
We report the detection of carbon monoxide (CO) emission from the young supernova remnant Cassiopeia A (Cas A) at wavelengths corresponding to the fundamental vibrational mode at 4.65 micron. We obtained AKARI Infrared Camera spectra towards 4 positi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::73bd3a44df3aa08b007ac15e93c9bf6a
Autor:
Jeonghee Rho, Karl Isensee, Haley Louise Gomez, J. D. T. Smith, William T. Reach, Lawrence Rudnick, Takashi Kozasa, Tracey DeLaney
We used the Spitzer Space Telescope's Infrared Spectrograph to create a high resolution spectral map of the central region of the Cassiopeia A supernova remnant, allowing us to make a Doppler reconstruction of its 3D structure. The ejecta responsible
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cd02e23c89a83fbb05953b8e9c6f69a0