Wolf–Rayet star

Results: 111



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41THE ASTROPHYSICAL JOURNAL, 502 : 833È846, 1998 August[removed]The American Astronomical Society. All rights reserved. Printed in U.S.A. TEMPORAL VARIATIONS OF MIDINFRARED SPECTRA IN LATE-TYPE STARS J. D. MONNIER,1 T.

THE ASTROPHYSICAL JOURNAL, 502 : 833È846, 1998 August[removed]The American Astronomical Society. All rights reserved. Printed in U.S.A. TEMPORAL VARIATIONS OF MIDINFRARED SPECTRA IN LATE-TYPE STARS J. D. MONNIER,1 T.

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Source URL: isi.ssl.berkeley.edu

Language: English - Date: 2005-06-13 13:51:52
42Mismatched Twin Stars Spotted in the Delivery Room2015-06 | www.cfa.harvard.edu/ CfA Home   HCO Home

Mismatched Twin Stars Spotted in the Delivery Room2015-06 | www.cfa.harvard.edu/ CfA Home   HCO Home

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Source URL: lsst.org

Language: English - Date: 2015-02-17 12:35:51
43Object-X : The Brightest Mid-IR Point Source in M33 Rubab Khan1 , K. Z. Stanek1,2 , C. S. Kochanek1,2 , A. Z. Bonanos3 arXiv:1012.3457v1 [astro-ph.SR] 15 Dec[removed]ABSTRACT

Object-X : The Brightest Mid-IR Point Source in M33 Rubab Khan1 , K. Z. Stanek1,2 , C. S. Kochanek1,2 , A. Z. Bonanos3 arXiv:1012.3457v1 [astro-ph.SR] 15 Dec[removed]ABSTRACT

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Source URL: arxiv.org

Language: English - Date: 2014-01-25 12:01:25
44fig. 1, D. Baade has plotted our observations of HR[removed]phase 0.5 eorresponds to the primary shell phase) and shows that there is no modulation of the light eurve with phase of the orbital period. Unfortunately the sho

fig. 1, D. Baade has plotted our observations of HR[removed]phase 0.5 eorresponds to the primary shell phase) and shows that there is no modulation of the light eurve with phase of the orbital period. Unfortunately the sho

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Source URL: www.eso.org

Language: English - Date: 2009-06-05 10:39:32
45e.g., the 10-9, 2.429t-tm, observed in other high excitation objects such as Wolf-Rayet stars (Aitken et al., 1982, Monthly Notices of the Royal Astronomical Society, 200, 698) are not present in our spectrum of the nova

e.g., the 10-9, 2.429t-tm, observed in other high excitation objects such as Wolf-Rayet stars (Aitken et al., 1982, Monthly Notices of the Royal Astronomical Society, 200, 698) are not present in our spectrum of the nova

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Source URL: www.eso.org

Language: English - Date: 2009-06-05 10:39:39
46We have observed E Cr A at the ESO 1 m telescope during the nights of July 213 and 3/4, 1982. The period 01 the system is 14 ~ [removed]and we have a large part 01 a complete cycle (a 12 hours run centred on the meridian

We have observed E Cr A at the ESO 1 m telescope during the nights of July 213 and 3/4, 1982. The period 01 the system is 14 ~ [removed]and we have a large part 01 a complete cycle (a 12 hours run centred on the meridian

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Source URL: www.eso.org

Language: English - Date: 2009-06-05 10:39:35
47The Hertzsprung-Russell Diagramm 1. Classifications of stars The spectrum of the brightest star, our Sun, shows several dark gaps perpendicular to the flow of it’s colours (figure 1). These so called spectral absorptio

The Hertzsprung-Russell Diagramm 1. Classifications of stars The spectrum of the brightest star, our Sun, shows several dark gaps perpendicular to the flow of it’s colours (figure 1). These so called spectral absorptio

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Source URL: www.aal.lu

Language: English - Date: 2001-06-17 17:07:28
48case we are now on the verge of seeing the birth of seismological investigation of non-variable stars. References Christensen-Dalsgaard, J., and Frandsen, S.: 1983, Solar Phys. 82, 469.

case we are now on the verge of seeing the birth of seismological investigation of non-variable stars. References Christensen-Dalsgaard, J., and Frandsen, S.: 1983, Solar Phys. 82, 469.

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Source URL: www.eso.org

Language: English - Date: 2009-06-05 10:39:38
49THE ASTROPHYSICAL JOURNAL, 511 : 721È729, 1999 February[removed]The American Astronomical Society. All rights reserved. Printed in U.S.A. ISO LWS SPECTROSCOPY OF M82 : A UNIFIED EVOLUTIONARY MODEL JAMES W. COLBERT,1,2

THE ASTROPHYSICAL JOURNAL, 511 : 721È729, 1999 February[removed]The American Astronomical Society. All rights reserved. Printed in U.S.A. ISO LWS SPECTROSCOPY OF M82 : A UNIFIED EVOLUTIONARY MODEL JAMES W. COLBERT,1,2

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Source URL: www.nrl.navy.mil

Language: English - Date: 2012-12-06 14:52:46
50Preprint typeset using LATEX style emulateapj v[removed]GCIRS16SW: A MASSIVE ECLIPSING BINARY IN THE GALACTIC CENTER ∗

Preprint typeset using LATEX style emulateapj v[removed]GCIRS16SW: A MASSIVE ECLIPSING BINARY IN THE GALACTIC CENTER ∗

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Source URL: orbi.ulg.ac.be

Language: English - Date: 2009-11-12 11:44:55