2.4 μm emission from the galactic centre region
✍ Scribed by A. W. Harris; D. Lemke; W. Hofmann
- Publisher
- Springer Netherlands
- Year
- 1980
- Tongue
- English
- Weight
- 530 KB
- Volume
- 72
- Category
- Article
- ISSN
- 0004-640X
No coin nor oath required. For personal study only.
📜 SIMILAR VOLUMES
A continuous monitoring of the Galactic Centre region has been performed with the WFC~s on board BeppoSAX on a time spread of about 7 months for a total of 500 ks exposure time. The long repeated observations allowed for the identification of 14 bursting sources, 2 of which uncataloged (SAXJ1750-290
From spectra recorded at a resolution of 0.020 cm 01 of the flame CH 4 / O 2 at low pressure, six new vibrational transitions in D£ 3 Å 1 with 2£ 1 / £ 2 Å 5 had been recently identified [ D. Bailly et al., J. Mol. Spectrosc. 182, 10 -17 ( 1996 ) ] based on the HITRAN 92 predictions. New calculation