Citation: O. Steiner et al., Radiative properties of magnetic elements - I. Why are G-band bright points bright?, ASTRON ASTR, 372(1), 2001, pp. L13-L16
Citation: Ph. Hauschildt et al., Parallel implementation of the Phoenix generalized stellar atmosphere program. III. A parallel algorithm for direct opacity sampling, ASTROPH J S, 134(2), 2001, pp. 323-329
Authors:
Albrow, M
Beaulieu, JP
Caldwell, JAR
Domink, M
Greenhill, J
Hill, K
Kane, S
Martin, R
Menzies, J
Pollard, K
Sackett, PD
Sahu, KC
Vermaak, P
Watson, R
Williams, A
Hauschildt, PH
Citation: M. Albrow et al., H alpha equivalent width variations across the face of a microlensed K giant in the galactic bulge, ASTROPHYS J, 550(2), 2001, pp. L173-L177
Authors:
Lentz, EJ
Baron, E
Lundqvist, P
Branch, D
Hauschildt, PH
Fransson, C
Garnavich, P
Bastian, N
Filippenko, AV
Kirshner, RP
Challis, PM
Jha, S
Leibundgut, B
McCray, R
Michael, E
Panagia, N
Phillips, MM
Pun, CSJ
Schmidt, B
Sonneborn, G
Suntzeff, NB
Wang, L
Wheeler, JC
Citation: Ej. Lentz et al., Analysis of type IInSN1998S: Effects of circumstellar interaction on observed spectra, ASTROPHYS J, 547(1), 2001, pp. 406-411
Authors:
Baron, E
Branch, D
Hauschildt, PH
Filippenko, AV
Kirshner, RP
Challis, PM
Jha, S
Chevalier, R
Fransson, C
Lundqvist, P
Garnavich, P
Leibundgut, B
McCray, R
Michael, E
Panagia, N
Phillips, MM
Pun, CSJ
Schmidt, B
Sonneborn, G
Suntzeff, NB
Wang, L
Wheeler, JC
Citation: E. Baron et al., Preliminary spectral analysis of the Type II supernova 1999em, ASTROPHYS J, 545(1), 2000, pp. 444-448
Citation: F. Allard et al., Spherically symmetric model atmospheres for low-mass pre-main-sequence stars with effective temperatures between 2000 and 6800 K, ASTROPHYS J, 539(1), 2000, pp. 366-371
Authors:
Basri, G
Mohanty, S
Allard, F
Hauschildt, PH
Delfosse, X
Martin, EL
Forveille, T
Goldman, B
Citation: G. Basri et al., An effective temperature scale for late-M and L dwarfs, from resonance absorption lines of CSI and RB I, ASTROPHYS J, 538(1), 2000, pp. 363-385
Citation: Ja. Orosz et Ph. Hauschildt, The use of the NEXTGEN model atmospheres for cool giants in a light curve synthesis code, ASTRON ASTR, 364(1), 2000, pp. 265-281