Add to ORKG[[sponsorship]]天文及天文物理研究所[[note]]已出版;[SCI];有審查制度;具代表性[[note]]http://gateway.isiknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Drexel&SrcApp=hagerty_opac&KeyRecord=0004-637X&DestApp=JCR&RQ=IF_CAT_BOXPLO
We report the discovery of water maser emission in eight active galactic nuclei (AGN) with the 70-m ...
The detection of 22 GHz water vapor emission from IC 342 is reported, raising the detection rate amo...
The young stellar object SVS 13 is believed to power the chain formed by the HH 7-11 objects. Recen...
[[abstract]]Using the Submillimeter Array (SMA) we have imaged for the first time the 321.226 GHz, 1...
[[sponsorship]]天文及天文物理研究所[[note]]已出版;[SCI];有審查制度;具代表性[[note]]http://gateway.isiknowledge.com/gateway...
SIGLEAvailable from British Library Document Supply Centre- DSC:D75664/87 / BLDSC - British Library ...
We report sensitive, high angular resolution VLA 3.6 cm and 7 mm continuum observations toward the s...
We present results from SMA observations of the star forming region Cepheus A-East at ~340 GHz (875 ...
Context. The 6.7 GHz methanol maser is exclusively associated with high-mass star formatio...
We report the first detection of an extragalactic millimeter wavelength H2O maser at 183 GHz towards...
Artículo de publicación ISIWe report continuum (1.3 cm) and H maser line observations, made with the...
[[sponsorship]]天文及天文物理研究所[[note]]已出版;[SCI];有審查制度;具代表性[[note]]http://gateway.isiknowledge.com/gateway...
Artículo de publicación ISIAt angular resolution of approximately 1 arc second(s) the Cepheus A East...
Submillimeter Array (SMA) Newsletter July 2015 Blundell, Raymond Submillimeter Array Newsletter |...
We compare the number of detected 22 GHz H2O masers in the Local Group galaxies M 31, M 33, NGC 682...
We report the discovery of water maser emission in eight active galactic nuclei (AGN) with the 70-m ...
The detection of 22 GHz water vapor emission from IC 342 is reported, raising the detection rate amo...
The young stellar object SVS 13 is believed to power the chain formed by the HH 7-11 objects. Recen...
[[abstract]]Using the Submillimeter Array (SMA) we have imaged for the first time the 321.226 GHz, 1...
[[sponsorship]]天文及天文物理研究所[[note]]已出版;[SCI];有審查制度;具代表性[[note]]http://gateway.isiknowledge.com/gateway...
SIGLEAvailable from British Library Document Supply Centre- DSC:D75664/87 / BLDSC - British Library ...
We report sensitive, high angular resolution VLA 3.6 cm and 7 mm continuum observations toward the s...
We present results from SMA observations of the star forming region Cepheus A-East at ~340 GHz (875 ...
Context. The 6.7 GHz methanol maser is exclusively associated with high-mass star formatio...
We report the first detection of an extragalactic millimeter wavelength H2O maser at 183 GHz towards...
Artículo de publicación ISIWe report continuum (1.3 cm) and H maser line observations, made with the...
[[sponsorship]]天文及天文物理研究所[[note]]已出版;[SCI];有審查制度;具代表性[[note]]http://gateway.isiknowledge.com/gateway...
Artículo de publicación ISIAt angular resolution of approximately 1 arc second(s) the Cepheus A East...
Submillimeter Array (SMA) Newsletter July 2015 Blundell, Raymond Submillimeter Array Newsletter |...
We compare the number of detected 22 GHz H2O masers in the Local Group galaxies M 31, M 33, NGC 682...
We report the discovery of water maser emission in eight active galactic nuclei (AGN) with the 70-m ...
The detection of 22 GHz water vapor emission from IC 342 is reported, raising the detection rate amo...
The young stellar object SVS 13 is believed to power the chain formed by the HH 7-11 objects. Recen...