Farihi, J; Becklin, EE; Macintosh, BA; (2004) Mid-Infrared Observations of van Maanen 2: No Substellar Companion. The Astrophysical Journal , 608 (2) L109-L112. 10.1086/422502.

Preview

Text Farihi_18331.web.pdf Download (146kB) | Preview

Abstract

The results of a comprehensive infrared imaging search for the putative 0.06 M☉ astrometric companion to the 4.4 pc white dwarf van Mannen 2 are reported. Adaptive optics images acquired at 3.8 μm reveal a diffraction-limited core of 0farcs09 and no direct evidence of a secondary. Models predict that at 5 Gyr, a 50MJ brown dwarf would be only 1 mag fainter than van Maanen 2 at this wavelength, and the astrometric analysis suggested a separation of 0farcs2. In the case of a chance alignment along the line of sight, a 0.4 mag excess should be measured. An independent photometric observation at the same wavelength reveals no excess. In addition, there exist published Infrared Space Observatory observations of van Maanen 2 at 6.8 and 15.0 μm that are consistent with the photospheric flux of a 6750 K white dwarf. If recent brown dwarf models are correct, there is no substellar companion with Teff gsim 500 K.

Download activity - last month

Export as CSVJSONXML

Download activity - last 12 months

Export as XMLJSONCSV

Downloads by country - last 12 months

Export as CSVJSONXML

Archive Staff Only

View Item