| Issue |
A&A
Volume 426, Number 2, November I 2004
|
|
|---|---|---|
| Page(s) | 523 - 534 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361:20035880 | |
| Published online | 11 October 2004 | |
The hot core-ultracompact H II connection in G10.47+0.03*
1
Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany e-mail: pascucci@mpia.de
2
Thüringer Landessternwarte Tautenburg, Sternwarte 5, 07778 Tautenburg, Germany
3
Leiden Observatory, PO Box 9513, 2300 RA Leiden, The Netherlands
Received:
16
December
2003
Accepted:
30
June
2004
We present infrared imaging and spectroscopic data of the complex
massive star-forming region G10.47+0.03.
The detection of seven mid-infrared (MIR) sources in our field
combined with a sensitive Ks/ISAAC image allows to establish a very
accurate astrometry, at the level of 0
3.
Two MIR sources are found to be coincident with two ultracompact regions
(s) within our astrometric accuracy.
Another MIR source lies very close to three other regions and to the
hot molecular core (HMC) in G10.47+0.03.
Spectroscopy of two of the most interesting MIR sources allows to identify the
location and spectral type of the ionizing sources.
We discuss in detail the relationship between the HMC, the regions and
the nearby MIR source. The nature of the other MIR sources is also investigated.
Key words: ISM: regions / infrared: stars / stars: individual: G10.47+0.03 / stars: formation
© ESO, 2004
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