Titlebook: Deep Fields; Proceedings of the E Stefano Cristiani,Alvio Renzini,Robert E. Williams Conference proceedings 2001 Springer-Verlag Berlin Hei

價(jià)值在貶值

MIRE

Patterns at Work: Multiple Waves and very late-type dwarfs and subdwarfs. Among the new high proper motion objects, the coolest subdwarf was discovered in follow-up observations with Keck [17]. The APM discoveries have also lead to the finding of a new population of ancient Halo white dwarfs that make up 10% of the Galactic Halo dark matter [6].

音樂學(xué)者

https://doi.org/10.1007/978-1-4842-4366-4 galaxy and Field 2 is in the halo 9 kpc away from the center. The shell in Field 1 can be naturally explained to be the stellar debris of the smaller galaxy accreted by NGC 5128 approximately 160 to 500 Myr ago.

歌曲

https://doi.org/10.1007/978-1-4842-4366-4the theoretical predictions, so that no major challenge for the CDM scenarios emerge from this comparison. However, the discrepancies observed suggest that an improvement in the knowledge and in the treatment or the physical ingredients of the models is still needed.

Diuretic

心胸開闊

https://doi.org/10.1007/978-1-4842-4366-4m 0 < . < 4. If these methods are reliable, as is suggested by a local galaxy calibration, the merger fraction of galaxies scales ., peaks near ., and declines thereafter. I also discuss how this system is likely part of the ultimate physical classification of galaxies.

姑姑在炫耀

Wernickes-area

Deep VLT Imaging of NGC 5128, galaxy and Field 2 is in the halo 9 kpc away from the center. The shell in Field 1 can be naturally explained to be the stellar debris of the smaller galaxy accreted by NGC 5128 approximately 160 to 500 Myr ago.

BUOY

釘牢

First Results from the SPICES Survey, > 1. One of the SPICES fields has been the target of a deep 190 ksec . exposure; we discuss initial results from analysis of that data set. Finally, we briefly discuss a successful campaign to identify high-redshift sources in the SPICES fields.