Zobrazeno 1 - 10
of 26
pro vyhledávání: '"Jeonghee Rho"'
Autor:
Jeonghee Rho, Aravind P Ravi, Le Ngoc Tram, Thiem Hoang, Jérémy Chastenet, Matthew Millard, Michael J Barlow, Ilse De Looze, Haley L Gomez, Florian Kirchschlager, Loretta Dunne
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 522:2279-2296
We present polarization observations of the young supernova remnant (SNR) Cas A using the High-resolution Airborne Wideband Camera-Plus (HAWC+) instrument onboard the Stratospheric Observatory for Infrared Astronomy (SOFIA). The polarization map at 1
Autor:
Mikako Matsuura, Roger Wesson, Richard G Arendt, Eli Dwek, James M De Buizer, John Danziger, Patrice Bouchet, M J Barlow, Phil Cigan, Haley L Gomez, Jeonghee Rho, Margaret Meixner
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 517:4327-4336
At a distance of 50 kpc, Supernova 1987A is an ideal target to study how a young supernova (SN) evolves in time. Its equatorial ring, filled with material expelled from the progenitor star about 20,000 years ago, has been engulfed with SN blast waves
Autor:
Jeonghee Rho, Haley Louise Gomez, Mikako Matsuura, Loretta Dunne, I. De Looze, Alberto Noriega-Crespo, Andreas Papageorgiou, F. D. Priestley, H. Chawner, M. J. Barlow, A. D. P. Howard, Matthew Smith, K. 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 present complicated dust structures within multiple regions of the candidate supernova remnant (SNR) the `Tornado' (G357.7-0.1) using observations with Spitzer and Herschel. We use Point Process Mapping, PPMAP, to investigate the distribution of d
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 Our sample includes previously unpublished profiles of lin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
Autor:
S. Valenti, Jeonghee Rho, Zhihao Chen, Lluís Galbany, J. Vinko, Sergei Blinnikov, R. Szakats, L. Kriskovics, Vishal Joshi, S. D. Van Dyk, A. Pal, Sung-Chul Yoon, Melissa L. Graham, Peter Hoeflich, Dipankar Banerjee, Melissa Shahbandeh, Jie Zhang, M. Williamson, A. Ordasi, H. Cha, A. Evans, Jamison Burke, M. Modjaz, C. McCully, X. F. Wang, Xue Li, H. Jin, Thomas R. Geballe, J. E. Andrews, H. An, C. Pellegrino, Daichi Hiramatsu, D. A. Howell, K. Vida, R. Cartier, T. Pritchard, S. Yan
Publikováno v:
The Astrophysical Journal
We present near-infrared and optical observations of the Type Ic Supernova (SN) 2020oi in the galaxy M100 and the broad-lined Type Ic SN2020bvc in UGC 9379, using Gemini, LCO, SOAR, and other ground-based telescopes. The near-IR spectrum of SN2020oi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::14ec9afc2e34483b153a225cb981258d
http://arxiv.org/abs/2010.00662
http://arxiv.org/abs/2010.00662
Autor:
Kevin Grieve, M. Lakicevic, Gavin Rowell, Kisetsu Tsuge, Akiko Kawamura, Kengo Tachihara, Tsuyoshi Inoue, Miroslav Filipovic, Knox S. Long, Shu-ichiro Inutsuka, Jeonghee Rho, F. Voisin, Norikazu Mizuno, Yasuo Fukui, T. Nagaya, Tea Temim, Sangwook Park, K. Fujii, Hidetoshi Sano, Lister Staveley-Smith, J. Th. van Loon, Remy Indebetouw, Satoshi Yoshiike, J. Seok, Y. Yamane, Toshikazu Onishi, Kazuki Tokuda
N49 (LHA 120-N49) is a bright X-ray supernova remnant (SNR) in the Large Magellanic Cloud. We present new $^{12}$CO($J$ = 1-0, 3-2), HI, and 1.4 GHz radio-continuum observations of the SNR N49 using Mopra, ASTE, ALMA, and ATCA. We have newly identifi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3f5bf580a0387b9ef1f26ea09428e2f5
http://arxiv.org/abs/1806.10390
http://arxiv.org/abs/1806.10390
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