Search Publications

The peculiar variable V838 Mon
DOI: 10.1046/j.1365-8711.2002.06017.x Bibcode: 2002MNRAS.336L..43K

Kimeswenger, S.; Lederle, C.; Schmeja, S. +1 more

V838 Mon underwent, after a first nova-like outburst in January and a usual decline, a second outburst after one month, and a third weak one again a month later. Moreover, a very small increase of the temperature at the beginning of April gives us a hint about a physical process with a period of one month. We obtained a BVRIC time-seque…

2002 Monthly Notices of the Royal Astronomical Society
eHST 79
The percentage of stellar light re-radiated by dust in late-type Virgo Cluster galaxies
DOI: 10.1046/j.1365-8711.2002.05881.x Bibcode: 2002MNRAS.335L..41P

Tuffs, Richard J.; Popescu, Cristina C.

We show that the mean percentage of stellar light re-radiated by dust is ~30 per cent for the Virgo Cluster late-spirals measured with ISOPHOT by Tuffs et al. A strong dependence of this ratio with morphological type was found, ranging from typical values of ~15 per cent for early spirals to up to ~50 per cent for some late spirals. The extreme BC…

2002 Monthly Notices of the Royal Astronomical Society
ISO 79
A new method for ISOCAM data reduction - II. Mid-infrared extragalactic source counts in the ELAIS Southern field
DOI: 10.1046/j.1365-8711.2002.05672.x Bibcode: 2002MNRAS.335..831G

Pozzi, F.; Franceschini, A.; Serjeant, S. +5 more

We present the 15-µm extragalactic source counts from the Final Analysis Catalogue of the European Large Area ISO Survey (ELAIS) Southern hemisphere field S1, extracted using the Lari method. The large number of extragalactic sources (~350) detected over this area between about 0.5 and 100 mJy guarantee a high statistical significance of the…

2002 Monthly Notices of the Royal Astronomical Society
ISO 77
Circumnuclear regions in barred spiral galaxies - II. Relations to host galaxies
DOI: 10.1046/j.1365-8711.2002.05840.x Bibcode: 2002MNRAS.337..808K

Knapen, J. H.; Pérez-Ramírez, D.; Laine, S.

We present optical broad- and narrow-band imaging of a sample of a dozen barred galaxies. These images are analysed in conjunction with our previously published near-infrared imaging of their central regions and with literature values for, e.g. bar strengths and the total star formation activity of the galaxies. We present B, I and Hα images, and …

2002 Monthly Notices of the Royal Astronomical Society
eHST 73
A Hubble Space Telescope lensing survey of X-ray-luminous galaxy clusters - II. A search for gravitationally lensed EROs *
DOI: 10.1046/j.1365-8711.2002.04984.x Bibcode: 2002MNRAS.330....1S

Kneib, J. -P.; Ivison, R. J.; Smith, Graham P. +7 more

We present the results of a survey for extremely red objects (EROs) undertaken in the fields of 10 massive galaxy cluster lenses at , combining sensitive, high-resolution Hubble Space Telescope imaging with deep, half-arcsecond K -band imaging from UKIRT. We detect 60 EROs with , of which 26 have in a total image-plane survey area of 49arcmin

2002 Monthly Notices of the Royal Astronomical Society
eHST 72
K dwarfs and the chemical evolution of the solar cylinder
DOI: 10.1046/j.1365-8711.2002.05825.x Bibcode: 2002MNRAS.336..879K

Chiappini, Cristina; Matteucci, Francesca; Flynn, Chris +1 more

K dwarfs have lifetimes older than the present age of the Galactic disc, and are thus ideal stars for investigating the chemical evolution of the disc. We have developed several photometric metallicity indicators for K dwarfs, based on a sample of accurate spectroscopic metallicities for 34 disc and halo G and K dwarfs. The photometric metalliciti…

2002 Monthly Notices of the Royal Astronomical Society
Hipparcos 69
Mass segregation in young compact star clusters in the Large Magellanic Cloud - I. Data and luminosity functions
DOI: 10.1046/j.1365-8711.2002.05217.x Bibcode: 2002MNRAS.331..228D

de Grijs, R.; Gilmore, G. F.; Johnson, R. A. +1 more

We have undertaken a detailed analysis of HST/WFPC2 and STIS imaging observations, and of supplementary wide-field ground-based observations obtained with the ESO New Technology Telescope (NTT) of two young (~10-25Myr) compact star clusters in the LMC, NGC 1805 and 1818. The ultimate goal of our work is to improve our understanding of the degree o…

2002 Monthly Notices of the Royal Astronomical Society
eHST 68
Echoes in X-ray binaries
DOI: 10.1046/j.1365-8711.2002.05530.x Bibcode: 2002MNRAS.334..426O

Horne, Keith; O'Brien, K.; Chen, W. +3 more

We present a method of analysing the correlated X-ray and optical/UV variability in X-ray binaries, using the observed time delays between the X-ray driving light curves and their reprocessed optical echoes. This allows us to determine the distribution of reprocessing sites within the binary. We model the time-delay transfer functions by simulatin…

2002 Monthly Notices of the Royal Astronomical Society
eHST 68
Mass segregation in young compact clusters in the Large Magellanic Cloud - III. Implications for the initial mass function
DOI: 10.1046/j.1365-8711.2002.05954.x Bibcode: 2002MNRAS.337..597D

Santiago, B. X.; Mackey, A. D.; de Grijs, R. +4 more

The distribution of core radii of rich clusters in the Large Magellanic Cloud (LMC) systematically increases in both upper limit and spread with increasing cluster age. Cluster-to-cluster variations in the stellar initial mass function (IMF) have been suggested as an explanation. We discuss the implications of the observed degree of mass segregati…

2002 Monthly Notices of the Royal Astronomical Society
eHST 67
The SCUBA 8-mJy survey - II. Multiwavelength analysis of bright submillimetre sources
DOI: 10.1046/j.1365-8711.2002.05111.x Bibcode: 2002MNRAS.331..839F

Ivison, R. J.; Dunlop, J. S.; Serjeant, S. +13 more

We present the results of a multiwavelength study of the 19 most significant submillimetre (submm) sources detected in the SCUBA 8-mJy survey. As described in Scott et al. , this survey covers ~=260arcmin2 using the submillimetre camera SCUBA, to a limiting source detection limit S 850µm ~=8mJy. One advantage of this re…

2002 Monthly Notices of the Royal Astronomical Society
ISO 66