The present-day chemical composition of the LMC

WRJ Rolleston, C Trundle, PL Dufton - Astronomy & Astrophysics, 2002 - aanda.org
High-resolution observations of five OB-type main-sequence stars in the Large Magellanic
Cloud (LMC) have been obtained with the UCL échelle spectrograph on the 3.9-m Anglo …

B-type supergiants in the SMC: Chemical compositions and comparison of static and unified models

PL Dufton, RSI Ryans, C Trundle, DJ Lennon… - Astronomy & …, 2005 - aanda.org
High-resolution UCLES/AAT spectra are presented for nine B-type supergiants in the SMC,
chosen on the basis that they may show varying amounts of nuclear-synthetically processed …

The chemical composition of the young, Inter-Cloud population

WRJ Rolleston, PL Dufton… - … and Astrophysics, v …, 1999 - adsabs.harvard.edu
High-resolution AAT spectroscopy and lower resolution spectrophotometry are presented for
three early B-type stars that are members of the young, Inter-Cloud population between the …

[HTML][HTML] Cool prominences in the corona of the rapidly rotating dMe star, HK Aquarii.

PB Byrne, MT Eibe… - … and Astrophysics, v. 311, p …, 1996 - adsabs.harvard.edu
Cool prominences in the corona of the rapidly rotating dMe star, HK Aquarii. ADS Classic is now
deprecated. It will be completely retired in October 2019. This page will automatically redirect to …

Chemical compositions of four B-type supergiants in the SMC wing

JK Lee, WRJ Rolleston, PL Dufton… - Astronomy & …, 2005 - aanda.org
High-resolution UCLES/AAT spectra of four B-type supergiants in the SMC South East Wing
have been analysed using non-LTE model atmosphere techniques to determine their …

Prominence and plage activity in the recently discovered late-type rapid rotator, RE 1816+ 541

MT Eibe - Astronomy and Astrophysics, v. 337, p. 757-771 …, 1998 - adsabs.harvard.edu
The rapidly-rotating, chromospherically active late-type star RE 1816+ 541 has shown signs
of intense magnetic activity in various forms. Time-series of high resolution spectra have …

Metallicity and photospheric abundances in field K and M dwarfs

M Zboril, PB Byrne - Monthly Notices of the Royal Astronomical …, 1998 - academic.oup.com
Elemental abundances in late-type stars are of interest in several ways: they determine the
location of the stars in the HR diagram and therefore their ages, as well as the atmospheric …

Evidence for large-scale, global mass inflow and flaring on the late-type fast rotator BD+ 22 deg 4409

MT Eibe, PB Byrne, RD Jeffries… - … v. 341, p. 527-538 (1999 …, 1999 - adsabs.harvard.edu
We present new results from high-resolution spectroscopic observations of the late-type fast
rotator BD+ 22 () deg4409, revealing interesting aspects about its magnetic activity that have …

Early-type stars in the Galactic halo from the Palomar-Green Survey II: A sample of distant, apparently young Population I stars

WRJ Rolleston, NC Hambly, FP Keenan… - … and Astrophysics, v …, 1999 - adsabs.harvard.edu
We present échelle (R~ 40 000) spectroscopic observations for a sample of apparently
normal, high Galactic latitude, early-type stars drawn from the Palomar-Green Survey. The …

Lithium abundance in field K and M dwarfs

M Zboril, PB Byrne, W Rolleston - Monthly Notices of the Royal …, 1997 - academic.oup.com
It is widely accepted that lithium abundance in late-type stars correlates with other stellar
characteristics, such as age, chromospheric activity and rotation. for example, the post-main …