Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.251..303p&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 251, July 15, 1991, p. 303-309. Research supported by A
Astronomy and Astrophysics
Astronomy
40
Dark Matter, Infrared Astronomy, Nebulae, Pre-Main Sequence Stars, Star Formation, Carbon Dioxide, Herbig-Haro Objects, Infrared Astronomy Satellite, Molecular Gases, Protostars, Red Shift, Stellar Mass
Scientific paper
IRAS Pointed Observations are used to study the premain sequence (PMS) objects associated with the reflection nebula Cederblad 110 in the Chamaeleon I star forming cloud. Nine PMS stars are identified, and near-infrared observations are presented and combined with IRAS data to investigate their evolutionary status. The nine objects represent various low-mass PMS stages from deeply embedded protostar candidates to naked T Tauri stars approaching the ZAMS, indicating that star formation has been going on for millions of years in the immediate vicinity of Cederblad 110. The two youngest PMS objects, Ced 110 IRS4 and Ced 110 IRS6, are projected on to the densest gas of the Chamaeleon I cloud suggesting an ongoing star formation process in the Cederblad 110 region.
Clark Frank O.
Laureijs Rene J.
Prusti Timo
Whittet Doug C. B.
Zhang Cheng-Yong
No associations
LandOfFree
A study of the Chamaeleon I dark cloud and T-association. IV - Infrared objects near Cederblad 110 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A study of the Chamaeleon I dark cloud and T-association. IV - Infrared objects near Cederblad 110, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A study of the Chamaeleon I dark cloud and T-association. IV - Infrared objects near Cederblad 110 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-863439