Zobrazeno 1 - 10
of 53
pro vyhledávání: '"John B. Whiteoak"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 409:371-388
We present molecular-line observations at millimetre, centimetre and infrared wavelengths of the region containing OH(1720 MHz) masers in the supernova remnant (SNR) G349.7+0.2, using the Australia Telescope (AT) Mopra antenna, the Swedish-ESO Submil
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c10ff637c651b6223a3fd4f065d04cd1
https://doi.org/10.1111/j.1365-2966.2010.17315.x
https://doi.org/10.1111/j.1365-2966.2010.17315.x
Publikováno v:
The Astrophysical Journal. 649:224-234
We present aperture synthesis imaging of dense molecular gas in the Large Magellanic Cloud, taken with the prototype millimeter receivers of the Australia Telescope Compact Array (ATCA). Our observations of the N113 HII region reveal a condensation w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fd78767a6c8adc12d2c712b11d512069
https://doi.org/10.1086/504968
https://doi.org/10.1086/504968
Autor:
Maria Cunningham, John B. Whiteoak
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 364:37-46
The 3-mm transitions of HCN, HCO + and HNC in the dense molecular clouds near the nucleus of the southern starburst galaxy NGC 4945 have been observed with three antennas of the Australia Telescope Compact Array (ATCA). Molecular-line emission was de
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7a4d8d83fdfbe4a6107df0cff580f361
https://doi.org/10.1111/j.1365-2966.2005.09502.x
https://doi.org/10.1111/j.1365-2966.2005.09502.x
Autor:
Maria R. Hunt, John B. Whiteoak
Publikováno v:
Astrophysics and Space Science. 295:257-262
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c73eb30300af6dfacee7ae7588d99afa
https://doi.org/10.1007/s10509-005-3701-2
https://doi.org/10.1007/s10509-005-3701-2
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 347:1164-1172
The VLA was used to determine precise positions for 4765-MHz OH maser emission sources toward star-forming regions which had been observed about seven months earlier with the Effelsberg 100-meter telescope. The observations were successful for K3-50,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a8049d2688ffbf2eed101eb1e1da8373
https://doi.org/10.1111/j.1365-2966.2004.07280.x
https://doi.org/10.1111/j.1365-2966.2004.07280.x
Publikováno v:
Proceedings of the Galactic Center Workshop 2002: The Central 300 parsecs of the Milky Way
The OH distribution in the Sgr A Complex has been observed in the 1612, 1665, 1667, and 1720 MHz OH transitions with the Very Large Array (VLA), in the BnA and DnC configurations. Spectral line maps have been produced with a channel velocity resoluti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::46a30fe6c3f5dfefa701d541bbde3bed
https://doi.org/10.1002/asna.200385033
https://doi.org/10.1002/asna.200385033
Publikováno v:
Astronomy & Astrophysics. 403:1011-1021
The OH distribution in the Sgr A Complex has been observed in the 1612-, 1665-, 1667- and 1720-MHz OH transitions with the Very Large Array (VLA) in BnA configuration. Maps are presented with a channel velocity resolution of about 9 km s -1 and with
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e7ed6c9a5073a52eb93cdd5e829f9dd4
https://doi.org/10.1051/0004-6361:20030309
https://doi.org/10.1051/0004-6361:20030309
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 331:969-974
ABSTRA C T Positions with subarcsecond accuracy have been measured for seven 22-GHz H2O masers associated with H II regions in the Large Magellanic Cloud (LMC); two of the masers are new detections. Initial position measurements were obtained with th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ae5bf8d429c68c758d621d00834c6c95
https://doi.org/10.1046/j.1365-8711.2002.05251.x
https://doi.org/10.1046/j.1365-8711.2002.05251.x
Autor:
Mark Wardle, John B. Whiteoak, Michael G. Burton, Jasmina Lazendic, A. J. Green, Michael C. B. Ashley, F. Yusef-Zadeh
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 331:537-544
We have found a bar of shocked molecular hydrogen (H2) towards the OH(1720 MHz) maser located at the projected intersection of supernova remnant (SNR) G359.1–0.5 and the nonthermal radio filament, known as the Snake. The H2 bar is well aligned with
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::93a7baa564918cf7f0e2bad7af5890ae
https://doi.org/10.1046/j.1365-8711.2002.05227.x
https://doi.org/10.1046/j.1365-8711.2002.05227.x
Autor:
Oskari Miettinen, R. S. Sault, Miikka S. Väisälä, C. M. Walmsley, John B. Whiteoak, M. J. Mantere, Jorma Harju
Cha-MMS1 was mapped in the NH_3(1,1) line and the 1.2 cm continuum using the Australia Telescope Compact Array, ATCA. The angular resolution of the ATCA observations is 7'' (~ 1000 AU), and the velocity resolution is 50 m s^{-1}. The core was also ma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9b9916774924cf7ba4fe66fd92986204
https://aaltodoc.aalto.fi/handle/123456789/32946
https://aaltodoc.aalto.fi/handle/123456789/32946
