Abstract
Using simple infrared color selection, the Two Micron All Sky Survey (2MASS) has found a large number of red, previously unidentified, radio-quiet quasi-stellar objects (QSOs). Although missed by UV/optical surveys, the 2MASS QSOs have Ks-band luminosities that are comparable to "classical" QSOs. This suggests the possible discovery of a previously predicted large population of dust-obscured radio-quiet QSOs. We present the results of an imaging survey of 29 2MASS QSOs observed with the Wide-Field Planetary Camera 2 on board the Hubble Space Telescope, I-band images, which benefit from the relative faintness of the nuclei at optical wavelengths, are used to characterize the host galaxies, measure the nuclear contribution to the total observed I-band emission, and survey the surrounding environments. The 2MASS QSOs are found to lie in galaxies with a variety of morphologies, luminosities, and dynamical states, not unlike those hosting radio-quiet Palomar-Green QSOs. Our analysis suggests that the extraordinary red colors of the 2MASS QSOs are caused by extinction of an otherwise typical QSO spectrum due to dust near the nucleus.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 707-729 |
| Number of pages | 23 |
| Journal | Astrophysical Journal |
| Volume | 590 |
| Issue number | 2 I |
| DOIs | |
| State | Published - Jun 20 2003 |
Keywords
- Dust, extinction
- Galaxies: active
- Galaxies: interactions
- Quasars: general
- Surveys
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science