Results 21 to 30 of about 753 (61)
The R136 star cluster hosts several stars whose individual masses
greatly exceed the accepted 150 Msun stellar mass limit [PDF]
, 2010 Spectroscopic analyses of H-rich WN5-6 stars within the young star clusters
NGC 3603 and R136 are presented, using archival HST & VLT spectroscopy, & high
spatial resolution near-IR photometry. We derive high T* for the WN stars in
NGC 3603 (T*~42+/-2 kK)Andersen, Anosova, Asplund, Binney, Blum, Bonanos, Bond, Brandl, Brandner, Bromm, Campbell, Cassinelli, Chlebowski, Clark, Conti, Crowther, Crowther, Crowther, Crowther, De Koter, De Koter, Drissen, Eggenberger, Eisenhauer, Espinoza, Esteban, Evans, Evans, Figer, Figer, Figer, Fitzpatrick, Frischknecht, Gal-Yam, Gibson, Goodwin, Guerrero, Harayama, Hasan Abu Kassim, Heap, Heger, Heger, Hillier, Hillier, Hirschi, Hunter, Hunter, Israel, Kim, Klapp, Koen, Kroupa, Lada, Lang, Langer, Langer, Lanz, Lebouteiller, Leitherer, Lejeune, Maeder, Martins, Maschberger, Massey, Massey, Massey, Massey, Massey, Massey, Maíz Apellániz, Melena, Meynet, Mills, Moffat, Moffat, Moffat, Moffat, Mokiem, Niemela, Norhasliza Yusof, Nugis, Oey, Ofek, Olivier Schnurr, Parker, Paul A. Crowther, Peimbert, Pittard, Pittard, Portegies Zwart, Puls, Raphael Hirschi, Rauw, Rauw, Reid, Reyes-Iturbide, Richard J. Parker, Ruehling, Russell, Rühling, Savage, Schmutz, Schnurr, Schnurr, Schnurr, Selman, Simon P. Goodwin, Skrutskie, Smith, Smith, Stevens, Stolte, Sung, Townsley, Vazquez, Vink, Walborn, Walborn, Walborn, Wang, Weidner, Weidner, Weigelt, Wolff, Yoon, Zinnecker +125 morecore +3 more sourcesThe Massive Star-forming Regions Omnibus X-ray Catalog [PDF]
, 2014 We present the Massive Star-forming Regions (MSFRs) Omnibus X-ray Catalog
(MOXC), a compendium of X-ray point sources from {\em Chandra}/ACIS
observations of a selection of MSFRs across the Galaxy, plus 30 Doradus in the
Large Magellanic Cloud.Bouwman, Jeroen, Broos, Patrick S., Feigelson, Eric D., Garmire, Gordon P., Getman, Konstantin V., Kuhn, Michael A., Povich, Matthew S., Townsley, Leisa K. +7 morecore +1 more sourceThe Onfp Class in the Magellanic Clouds [PDF]
, 2010 The Onfp class of rotationally broadened, hot spectra was defined some time
ago in the Galaxy, where its membership to date numbers only eight. The
principal defining characteristic is a broad, centrally reversed He II
$\lambda$4686 emission profile ...Anthony F. J. Moffat, Ardeberg, Azzopardi, Bouret, Cecilia Fariña, Christopher J. Evans, Crowther, Fariña, Gray, Guillermo L. Bosch, Heap, Henrichs, Howarth, Ian D. Howarth, Isserstedt, Isserstedt, Jacco Th. van Loon, Kendall, Kendall, Langer, Lanz, Lennon, Mason, Massey, Massey, Maíz Apellániz, Nicole St-Louis, Nidia I. Morrell, Nolan R. Walborn, Paul A. Crowther, Penny, Rodolfo H. Barbá, Sanduleak, Schild, Udalski, Walborn, Walborn, Walborn, Walborn, Walborn, Walborn, Zaritsky +41 morecore +3 more sourcesGravity-mode period spacings as seismic diagnostic for a sample of gamma
Doradus stars from Kepler space photometry and high-resolution ground-based
spectroscopy [PDF]
, 2015 Gamma Doradus stars (hereafter gamma Dor stars) are gravity-mode pulsators of
spectral type A or F. Such modes probe the deep stellar interior, offering a
detailed fingerprint of their structure.Aerts, C., Bloemen, S., De Smedt, K., Debosscher, J., Degroote, P., Fremat, Y., Fuentes, A. S., Homan, W., Hrudkova, M., Karjalainen, R., Lombaert, R., Nemeth, P., Oestensen, R., Papics, P. I., Raskin, G., Schmid, V. S., Tkachenko, A., Triana, S. A., Van De Steene, G., Van Reeth, T., Van Winckel, H., Vos, J., Zwintz, K. +22 morecore +2 more sourcesEta Carinae and the Luminous Blue Variables
, 2011 We evaluate the place of Eta Carinae amongst the class of luminous blue
variables (LBVs) and show that the LBV phenomenon is not restricted to
extremely luminous objects like Eta Car, but extends luminosities as low as
log(L/Lsun) = 5.4 - corresponding ...A Gal-Yam, A Herrero, A Nota, A Pasquali, A Pastorello, AF Valeev, AJ Marle van, AM Genderen van, AM Soderberg, B Davies, B Davies, B Davies, B Wolf, C Buemi, C Jager de, C Jager de, C Leitherer, C Sterken, C Sterken, C Sterken, C Trundle, C Trundle, DC Abbott, DJ Hillier, DJ Hillier, DJ Hillier, DJ Lennon, E Berger, E. Hubble, F Martins, F Najarro, F-J Zickgraf, G Meynet, G Umana, HE Bond, I Appenzeller, J Puls, JB Hutchings, JC Mauerhan, JH Groh, JH Groh, JH Groh, JH Groh, JH Guo, JI Castor, JL Prieto, JS Clark, JS Clark, JS Vink, JS Vink, JS Vink, K Davidson, K Davidson, K Davidson, K Lefever, K Weis, KH Nordsieck, LB Lucy, LB Lucy, LJ Smith, LR Yungelson, M Cantiello, M Groot de, M Patel, MT Botticella, N Langer, N Markova, N Markova, N Smith, N Smith, N Smith, N Smith, N Smith, N Smith, NR Walborn, O Stahl, O Stahl, O Stahl, O Stahl, P Benaglia, P Cox, P Massey, P Podsiadlowski, PA Crowther, PA Whitelock, PE Müller, R Boekel van, R Kotak, RB Stothers, RD Oudmaijer, RD Oudmaijer, RE Schulte-Ladbeck, RJ Foley, RM Humphreys, RM Humphreys, RM Humphreys, RM Humphreys, RM Humphreys, RM Humphreys, SA Pustilnik, SD Ryder, SE Woosley, SM White, T Zethson, TJ Harries, TJ Harries, TJ Jones, VV Dwarkadas, VV Gvaramadze, W Glatzel, W-R Hamann, WJ Wit de, YI Izotov +112 morecore +1 more sourceHD 51106 and HD 50747: an ellipsoidal binary and a triple system
observed with CoRoT
, 2009 We present an analysis of the observations of HD 51106 and HD 50747 by the
satellite CoRoT, obtained during its initial run, and of the spectroscopic
preparatory observations.A. Baglin, A. Hui-Bon-Hoa, Auvergne, C. Catala, D. Le Contel, Davidge, Donati, E. Michel, E. Poretti, G. Vauclair, Hauck, Henry, Henry, Ilijic, J.-C. Valtier, K. Uytterhoeven, Kurtz, Lehmann-Filhes, Lenz, Li, M. Auvergne, M. Rainer, Mathias, Moon, N. Dolez, O'Connell, P. J. Amado, P. Mathias, Piskunov, Poretti, R. Samadi, S. Vauclair, Solano, Vauclair +33 morecore +3 more sourcesOn Luminous Blue Variables as the Progenitors of Core-Collapse
Supernovae, especially Type IIn Supernovae
, 2010 Luminous blue variable (LBV) stars are very massive, luminous, unstable stars
that suffer frequent eruptions. In the last few years, these stars have been
proposed as the direct progenitors of some core-collapse supernovae (SNe),
particularly Type IIn ...Aldering, Anderson, Arthur, Balick, Bauer, Blondin, Chevalier, Chevalier, Chevalier, Chevalier, Chu, Chu, Chugai, Chugai, Chugai, Chugai, Chugai, Chugai, Crowther, Dwarkadas, Dwarkadas, Dwarkadas, Dwarkadas, Dwarkadas, Dwarkadas, Dwarkadas, Dwarkadas, Dwarkadas, Eldridge, Falk, Foley, Fox, Frank, Frank, Fransson, Freyer, Freyer, Gal-Yam, Gal-Yam, Garcia-Segura, Gräfener, Hamuy, Heger, Hirschi, Humphreys, Humphreys, Immler, Immler, Klein, Kotak, Kotak, Kwok, Langer, Langer, Levesque, Lundqvist, Maeder, Maeder, McCray, Miller, Morris, Pastorello, Pastorello, Podsiadlowski, Podsiadlowski, Podsiadlowski, Podsiadlowski, Puls, Puls, Ryder, Ryder, Salamanca, Salamanca, Schaller, Schlegel, Smartt, Smith, Smith, Smith, Smith, Smith, Smith, Smith, Soderberg, Sonneborn, Stockdale, Stothers, Tenorio-Tagle, Trundle, Trundle, ud-Doula, V. V. Dwarkadas, van Dyk, Vink, Vink, Vink, Weaver, Yoon +97 morecore +1 more source
