Universitat de - Departament d'Astronomia i Meteorologia ...
Universitat de - Departament d'Astronomia i Meteorologia ...
Universitat de - Departament d'Astronomia i Meteorologia ...
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172 General conclusions<br />
particular, runaway microquasars could be connected with some of the uni<strong>de</strong>n-<br />
tified faint, variable, and soft γ-ray EGRET sources above/below the galactic<br />
plane.<br />
Part II:<br />
1. We have presented a cross-i<strong>de</strong>ntification method to search for REXBs, which<br />
are potential microquasar sources. The obtained results give confi<strong>de</strong>nce to<br />
the proposed method, since the output list of objects inclu<strong>de</strong>d all but one<br />
known persistent HMXB microquasars within |b| < 5 ◦ . The obtained list<br />
after removing previously known sources contains 13 new radio emitting X-<br />
ray sources, of which 8 have been classified as high priority objects.<br />
2. We have studied 6 of these 8 sources, and found optical counterparts to all of<br />
them. We have obtained accurate positions at both radio and optical wave-<br />
lengths, perfectly compatible between them. We also have obtained radio<br />
spectra and optical magnitu<strong>de</strong>s of the sources.<br />
3. We have presented EVN and MERLIN observations of these six sources. Five<br />
of the six objects have been <strong>de</strong>tected and imaged, presenting different mor-<br />
phologies: one source has a two-si<strong>de</strong>d jet, three sources have one-si<strong>de</strong>d jets,<br />
and one source is compact.<br />
4. After our observations we conclu<strong>de</strong> that the sources 1RXS J001442.2+580201<br />
and 1RXS J013106.4+612035 are promising microquasar candidates in the<br />
Galaxy. 1RXS J042201.0+485610 is probably of thermal nature due to its<br />
highly inverted spectrum at high radio frequencies, and we note its exten<strong>de</strong>d<br />
appearance at optical wavelengths. 1RXS J062148.1+174736 is probably ex-<br />
tragalactic due to the exten<strong>de</strong>d optical counterpart. 1RXS J072259.5−073131<br />
displays a bent one-si<strong>de</strong>d jet, which is a common property in blazars. Finally,<br />
the source 1RXS J072418.3−071508 is an already i<strong>de</strong>ntified quasar.<br />
5. Work in progress. Optical spectroscopic observations of the first five sources<br />
are in progress for autumn 2002, to clearly unveil their galactic or extragalactic<br />
nature. On the other hand, the remaining sources in the list will be eventually<br />
studied in the future.