Large proper motions in the remarkable triple radio source in Serpens

1989 ◽  
Vol 346 ◽  
pp. L85 ◽  
Author(s):  
L. F. Rodriguez ◽  
S. Curiel ◽  
J. M. Moran ◽  
I. F. Mirabel ◽  
M. Roth ◽  
...  
Keyword(s):  
2012 ◽  
Vol 8 (S287) ◽  
pp. 103-107
Author(s):  
Tomoya Hirota ◽  
Masato Tsuboi ◽  
Kenta Fujisawa ◽  
Mareki Honma ◽  
Noriyuki Kawaguchi ◽  
...  

AbstractIn 2011 February, a burst of the 22 GHz H2O maser in Orion KL was reported. In order to identify the bursting maser features, we have been carrying out observations of the 22 GHz H2O maser in Orion KL with VERA, a Japanese VLBI network dedicated for astrometry. The bursting maser turns out to consist of two spatially different features at 7.58 and 6.95 km s−1. We determine their absolute positions and find that they are coincident with the shocked molecular gas called the Orion Compact Ridge. We tentatively detect the absolute proper motions of the bursting features toward the southwest direction, perpendicular to the elongation of the maser features. It is most likely that the outflow from the radio source I or another young stellar object interacting with Compact Ridge is a possible origin of the H2O maser burst. We will also carry out observations with ALMA in the cycle 0 period to monitor the submillimeter H2O maser lines in the Orion Compact Ridge region. These follow-up observations will provide novel information on the physical and chemical properties of the mastering region.


2020 ◽  
Vol 892 (2) ◽  
pp. 82 ◽  
Author(s):  
Luis F. Rodríguez ◽  
Sergio A. Dzib ◽  
Luis Zapata ◽  
Susana Lizano ◽  
Laurent Loinard ◽  
...  
Keyword(s):  

2005 ◽  
Vol 627 (1) ◽  
pp. L65-L68 ◽  
Author(s):  
Luis F. Rodríguez ◽  
Arcadio Poveda ◽  
Susana Lizano ◽  
Christine Allen
Keyword(s):  

2017 ◽  
Vol 834 (2) ◽  
pp. 140 ◽  
Author(s):  
Luis F. Rodríguez ◽  
Sergio A. Dzib ◽  
Laurent Loinard ◽  
Luis Zapata ◽  
Laura Gómez ◽  
...  

1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.


1978 ◽  
Vol 48 ◽  
pp. 389-390 ◽  
Author(s):  
Chr. de Vegt

AbstractReduction techniques as applied to astrometric data material tend to split up traditionally into at least two different classes according to the observational technique used, namely transit circle observations and photographic observations. Although it is not realized fully in practice at present, the application of a blockadjustment technique for all kind of catalogue reductions is suggested. The term blockadjustment shall denote in this context the common adjustment of the principal unknowns which are the positions, proper motions and certain reduction parameters modelling the systematic properties of the observational process. Especially for old epoch catalogue data we frequently meet the situation that no independent detailed information on the telescope properties and other instrumental parameters, describing for example the measuring process, is available from special calibration observations or measurements; therefore the adjustment process should be highly self-calibrating, that means: all necessary information has to be extracted from the catalogue data themselves. Successful applications of this concept have been made already in the field of aerial photogrammetry.


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