Hot-Star Group Publications, 1998

Hotty, the Group's Mascot

It's cool to be hot!


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1998

An optical and near-IR spectroscopic study of the extreme P Cygni-type supergiant HDE316285
D.J. Hillier, P.A. Crowther, F. Najarro, & A.W. Fullerton
A&A 340, 483 (1998)

Repetitive structure in the stellar wind of HD 93483: a normal O-type star
R.K. Prinja, D. Massa, I.D. Howarth & A.W. Fullerton.
MNRAS, 301, 926 (1998) (gzipped PostScript, 448kb)

HST UV measurements of wind structure and velocities in Local Group OB stars
R.K. Prinja, & P.A. Crowther
MNRAS, 300, 828 (1998)

Ejected Nebulae as Probes of the Evolution of Massive Stars in the Large Magellanic Cloud
L.J. Smith, A. Nota, A. Pasquali, C. Leitherer, M. Clampin & P.A. Crowther
ApJ 503, 278 (1998)

Microturbulence in O supergiants
K.C. Smith & I.D. Howarth
MNRAS, 299, 1146 (1998) (gzipped PostScript, 1.23Mb)

A spectropolarimetric survey of northern hemisphere Wolf-Rayet stars
T.J. Harries, D.J. Hillier, I.D. Howarth
MNRAS 296, 1072 (1998) (gzipped PostScript, 475kb)

Time-dependent structure in UV absorption lines of the rapid rotators HD 64760 (B0Ib) and HD 93521 (O9.5V)
I.D. Howarth, R.H. Townsend, M.J. Clayton, A.W. Fullerton, D.R. Gies, D. Massa, R.K. Prinja, A.H.N. Reid
MNRAS 296, 949 (1998)

Quantitative spectroscopy of Wolf-Rayet stars in HD97950 and R136a - the cores of giant HII regions
P.A.Crowther & L. Dessart
MNRAS 296, 622 (1998)

The WC10 central stars CPD-56 8032 and He2-113: II Model analysis and comparison with nebular properties
Orsola De Marco & P.A.Crowther
MNRAS 296, 419 (1998)

Quantitative classification of WC and WO stars
P.A.Crowther, Orsola De Marco, & M.J. Barlow
MNRAS 296, 367 (1998)

Clumping corrected mass-loss rates of Wolf-Rayet stars
T.Nugis, P.A.Crowther & A.J. Willis
A&A 333, 956 (1998)

Microturbulence in O supergiants
K.C. Smith, I.D.Howarth & K.W. Siebert
ASP Conference Series, Vol. 131, p. 153 (gzipped PostScript, 69kb)

Boulder-Munich II: Properties of Hot, Luminous Stars
I.D.Howarth (ed.)
(ASP Conference Series, Vol. 131)




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