Wavelengths of Fe ii lines for studies of time variation of the fine-structure constant

By Nave Gillian  

Monthly Notices of the Royal Astronomical Society, Vol. 420, Iss. 2, 2012-02 ,pp. : 1570-1574

Oxford University Press

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X-rays as the dominant excitation mechanism of [Fe ii] and H₂ emission lines in active galaxies

By Dors   Jr Oli L.   Riffel Rogemar A.   Cardaci Mónica V.   Hägele Guillermo F.   Krabbe Ângela C.   Pérez-Montero Enrique   Rodrigues Irapuan  

Monthly Notices of the Royal Astronomical Society, Vol. 422, Iss. 1, 2012-05 ,pp. : 252-260

Oxford University Press

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A large-scale structure traced by [O ii] emitters hosting a distant cluster at z= 1.62

By Tadaki Ken-ichi   Kodama Tadayuki   Ota Kazuaki   Hayashi Masao   Koyama Yusei   Papovich Casey   Brodwin Mark   Tanaka Masayuki   Iye Masanori  

Monthly Notices of the Royal Astronomical Society, Vol. 423, Iss. 3, 2012-07 ,pp. : 2617-2626

Oxford University Press

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Luminous [O iii] and [N ii] from tidally disrupted horizontal branch stars

By Clausen Drew   Sigurdsson Steinn   Eracleous Michael   Irwin Jimmy A.  

Monthly Notices of the Royal Astronomical Society, Vol. 424, Iss. 2, 2012-08 ,pp. : 1268-1274

Oxford University Press

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Evolution of the population of very strong Mg ii absorbers

By Rodríguez Hidalgo Paola   Wessels Kaylan   Charlton Jane C.   Narayanan Anand   Mshar Andrew   Cucchiara Antonino   Jones Therese  

Monthly Notices of the Royal Astronomical Society, Vol. 427, Iss. 3, 2012-12 ,pp. : 1801-1815

Oxford University Press

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