EXOr Variables as Seen in IR: on the Case of V1118 Ori

Details EXOr Variables as Seen in IR: on the Case of V1118 Ori EXOr Variables as Seen in IR: on the Case of V1118 Ori

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confe..27l&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 27-27"

Computer Science

Scientific paper

We have compiled the first EXOr catalogue containing all the IR (1-100 um) photometric and spectroscopic observations appeared in the literature during the last 30 years. By analyzing such catalogue, we present here some considerations about the relationship between the infrared observed properties of the EXOr variables and the mechanism(s) active during their evolutionary stage. Moreover, new results of our monitoring program based on near- and mid-IR photometry, near-IR spectroscopy and polarimetry of one object (V1118 Ori) typical of the class are presented and discussed in a coherent scheme. Our monitoring program (2005-2006) has covered part of the last outburst phase and the subsequent quiescent phase, providing some striking novelties (mainly spectroscopic). Clues are given in favour of interpreting the EXOr stage as following the FUOr one, more than to be a less evident manifestation of the same phase.

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