A grid of evolutionary synthesis models for different scenarios (initial mass function slope, metallicity, age, etc.) and computing a set of observables in a...
Multiwavelength Study of Star-Forming Galaxies in the Local Universe
We have studied in detail the properties of local active star-forming galaxies from the UCM survey, and in particular their star-formation histories. We have...
Near-infrared mapping of spiral galaxies. II - J, H, K profiles of M 31
Four radial profiles of M 31 in the near infrared taken with the 1.5 m infrared telescope of the Observatorio del Teide, Tenerife are presented. Three of these...
Neon and Chemical Fractionation Trends in Late-type Stellar Atmospheres
A survey of Ne, O and Fe coronal abundances culled from the recent literature for about 60 late-type stars confirms that the Ne/O ratio of stellar outer...
Neutral carbon and highly excited CO in a massive star-forming main sequence galaxy at z = 2.2
We used the Plateau De Bure Interferometer to observe multiple CO and neutral carbon transitions in a z = 2.2 main sequence disk galaxy, BX610. Our observation...
New insight into the T-type planetary mass population in the Sigma Orionis cluster
The proper characterization of the least massive population of the young Sigma Orionis star cluster is required to understand the form of the cluster mass...
New insights into a familiar friend - CO J = 2-1 mapping of the bipolar outflow source NGC 1333 (HH 7-11)
The bipolar outflow source NGC 1333 (HH 7-11) was observed in the J = 2-1 transition of (C-12)O, and evidence was found for a strong westerly termination of the...
New windows to the universe; Proceedings of the Eleventh IAU European Regional Astronomy Meeting, Universidad de La Laguna, Spain, July 3-8, 1989. Part III
Topics discussed in this issue include active galaxies and cosmology, interstellar and intergalactic medium, and astronomical instrumentation. Papers are...
NGC 1436: the making of a lenticular galaxy in the Fornax Cluster
We study the evolutionary path of the Fornax Cluster galaxy NGC 1436, which is known to be currently transitioning from a spiral into a lenticular morphology...