A&A 486, 533–544 (2008) Astronomy DOI: 10.1051/0004-6361:200809933 & c ESO 2008 Astrophysics The enigmatic young object: Walker 90/V590 Monocerotis, M. R. Pérez1, B. McCollum2,M.E.vandenAncker3, and M. D. Joner4 1 Los Alamos National Laboratory, PO Box 1663, ISR-1, MS B244, Los Alamos, NM 87545, USA e-mail:
[email protected] 2 Caltech, SIRTF Science Center, MS, 314-6, Pasadena, CA 91125, USA e-mail:
[email protected] 3 European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748, Garching bei München, Germany e-mail:
[email protected] 4 Brigham Young University, Dept. of Physics and Astronomy – ESC – N488, Provo, Utah 84602, USA e-mail:
[email protected] Received 8 April 2008 / Accepted 17 May 2008 ABSTRACT Aims. We assess the evolutionary status of the intriguing object Walker 90/V590 Mon, which is located about 20 arcmin northwest of the Cone Nebula near the center of the open cluster NGC 2264. This object, according to its most recent optical spectral type determination (B7), which we confirmed, is at least 3 mag too faint in V for the cluster distance, but it shows the classical signs of a young pre-main sequence object, such as highly variable Hα emission, Mg II emission, IR excess, UV continuum, and optical variability. Methods. We analyzed a collection of archival and original data on Walker 90, covering 45 years including photometry, imaging, and spectroscopic data ranging from ultraviolet to near-infrared wavelengths. Results. According to star formation processes, it is expected that, as this object clears its primordial surroundings, it should become optically brighter, show a weakening of its IR excess and present decreasing line emissions.