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Do we need to know the temperature in prestellar cores?PAVLYUCHENKOV, Ya; HENNING, Th; WIEBE, D et al.The Astrophysical journal. 2007, Vol 669, Num 2, issn 0004-637X, L101-L104, 2Article

The use of OH 'main' lines to constrain the variation of fundamental constantsKANEKAR, Nissim; CHENGALUR, J. N.Monthly Notices of the Royal Astronomical Society. 2004, Vol 350, Num 1, pp L17-L20, issn 0035-8711Article

FUSE OBSERVATIONS REVEAL THE NATURE OF THE STELLAR JETS IN R AqrNICHOLS, Joy; SLAVIN, Jonathan D.The Astrophysical journal. 2009, Vol 699, Num 1, pp 902-910, issn 0004-637X, 9 p., 1Article

MEASURED STARK WIDTHS OF SEVERAL Sn I AND Sn II SPECTRAL LINES IN A LASER-INDUCED PLASMAALONSO-MEDINA, A; COLON, C.The Astrophysical journal. 2008, Vol 672, Num 2, pp 1286-1291, issn 0004-637X, 6 p., 1Article

Dissociative shocks in the neighborhood of orion IRc2 traced with atomic carbonPARDO, Juan R; CERNICHARO, José; PHILLIPS, Thomas G et al.The Astrophysical journal. 2005, Vol 634, Num 1, pp L61-L64, issn 0004-637X, 2Article

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Ne II STARK WIDTH AND SHIFT REGULARITIESPELAEZ, R. J; DJUROVIC, S; CIRISAN, M et al.The Astrophysical journal. 2008, Vol 687, Num 2, pp 1423-1431, issn 0004-637X, 9 p., 1Article

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MULTIPLE COMPONENT OUTFLOWS IN AN ACTIVE REGION OBSERVED WITH THE EUV IMAGING SPECTROMETER ON HINODEBRYANS, P; YOUNG, P. R; DOSCHEK, G. A et al.The Astrophysical journal. 2010, Vol 715, Num 1, pp 1012-1020, issn 0004-637X, 9 p., 2Article

Forward modeling of hot loop oscillations observed by SUMER and SXTTAROYAN, Y; ERDELYI, R; WANG, T. J et al.The Astrophysical journal. 2007, Vol 659, Num 2, issn 0004-637X, L173-L176, 2Article

Are electric currents heating the magnetic chromosphere?SOCAS-NAVARRO, H.The Astrophysical journal. 2005, Vol 633, Num 1, pp L57-L60, issn 0004-637X, 2Article

On the transfer of resonant-line radiation in mesh simulationsTASITSIOMI, Argyro.The Astrophysical journal. 2006, Vol 648, Num 1, pp 762-766, issn 0004-637X, 5 p., 1Article

Simple formulae for estimating Stark widths and shifts of neutral atom linesDIMITRIJEVIC, M. S; KONJEVIC, N.Astronomy and astrophysics (Berlin. Print). 1986, Vol 163, Num 1-2, pp 297-300, issn 0004-6361Article

Variations of the asymmetry of disk-integrated solar line profilesBRUNING, D. H; LABONTE, B.Solar physics. 1985, Vol 97, Num 1, pp 1-7, issn 0038-0938Article

Stark broadening of ultraviolet Ar III spectral linesDJUROVIC, S; MAR, S; PELAEZ, R. J et al.Monthly notices of the Royal Astronomical Society (Print). 2011, Vol 414, Num 2, pp 1389-1396, issn 0035-8711, 8 p.Article

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MULTILINE SPECTROPOLARIMETRY OF THE QUIET SUN AT 5250 AND 6302 ÅSOCAS-NAVARRO, H; BORRERO, J. M; ASENSIO RAMOS, A et al.The Astrophysical journal. 2008, Vol 674, Num 1, pp 596-606, issn 0004-637X, 11 p., 1Article

THE ORIGIN OF RADIO SCINTILLATION IN THE LOCAL INTERSTELLAR MEDIUMLINSKY, Jeffrey L; RICKETT, Barney J; REDFIELD, Seth et al.The Astrophysical journal. 2008, Vol 675, Num 1, pp 413-419, issn 0004-637X, 7 p., 1Article

Simulation of quiet-sun waves in the Ca II infrared tripletPIETARILA, A; SOCAS-NAVARRO, H; BOGDAN, T et al.The Astrophysical journal. 2006, Vol 640, Num 2, pp 1142-1152, issn 0004-637X, 11 p., 1Article

SOLAR CYCLE VARIATION IN SUN-AS-A-STAR Can 854.2 nm BISECTORSPIETARILA, A; LIVINGSTON, W.The Astrophysical journal. 2011, Vol 736, Num 2, issn 0004-637X, 114.1-114.5, 1Article

Stark halfwidth trends along the homologous sequence of singly ionized noble gasesPELAEZ, R. J; DJUROVIC, S; CIRISAN, M et al.Astronomy and astrophysics (Berlin. Print). 2010, Vol 518, Num 2, issn 0004-6361, p. A60.1Article

Hβ PROFILES IN QUASARS : EVIDENCE FOR AN INTERMEDIATE-LINE REGIONCHEN HU; WANG, Jian-Min; HO, Luis C et al.The Astrophysical journal. 2008, Vol 683, Num 2, issn 0004-637X, L115-L118, 2Article