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G

Gargi Shaw

University System of Ohio

20H指数
72论文数
2.2K被引数
收录论文 30
发表时间
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Hydrodynamic Predictions for the Next Outburst of T Coronae Borealis: It Will Be the Brightest Classical or Recurrent Nova Ever Observed in X-RaysT Coronae Borealis下次爆发的流体动力学预测：它将是观测到的X射线波段最亮的经典新星或 recurrent nova。
errASTROPHYSICAL JOURNAL
IF5.4
err2025-03-19
err0
errOAAI
errStarrfield, S.; Bose, M.; Woodward, C. E.; Iliadis, C.; Hix, W. R.; Evans, A.; Shaw, G.; Banerjee, D. P. K.; Liimets, T.; Page, K. L.; Geballe, T. R.; Ilyin, I.; Perron, I.; Wagner, R. M.
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A spectrophotometric analysis and dust properties of classical nova V5584 Sgr
errMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
IF4.8
err2024-12-13
err0
errOAAI
errBisht, Mohit Singh; Raj, A.; Walter, F. M.; Bisht, D.; Shaw, Gargi; Belwal, K.; Biswas, S.
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XMM-Newton High-resolution Spectroscopy of EXO 0748-676 after Its Reemergence from a Long Quiescence
errASTROPHYSICAL JOURNAL LETTERS
IF11.7
err2024-12-03
err0
errOAAI
errBhattacharya, Sayantan; Bhattacharyya, Sudip; Shaw, Gargi
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A phenomenological study of the evolution of shock-induced O I emission lines in the spectrum of nova V2891 Cygni
errMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
IF4.8
err2024-07-13
err1
errOAAI
errPandey, Ruchi; Srivastava, Mudit K.; Shaw, Gargi
err分享
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A Photoionization Model for the Infrared Coronal Line Emission in the Classical Nova V1716 Scorpii
errASTROPHYSICAL JOURNAL
IF5.4
err2024-06-06
err3
errOAAI
errWoodward, C. E.; Shaw, G.; Starrfield, S.; Evans, A.; Page, K. L.
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Probing the tidal disruption event iPTF16axa with CLOUDY and disc-wind models
errMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
IF4.8
err2022-11-30
err2
errOAAI
errMageshwaran, T.; Shaw, Gargi; Bhattacharyya, Sudip
err分享
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Recent Updates to the Gas-phase Chemical Reactions and Molecular Lines in CLOUDY: Their Effects on Millimeter and Submillimeter Molecular Line Predictions
errASTROPHYSICAL JOURNAL
IF5.4
err2022-07-25
err3
errOAAI
errShaw, Gargi; Ferland, G. J.; Chatzikos, M.
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Detecting PAHs in high-z galaxies in proxy: modelling physical conditions in an extremely strong damped Lyman α absorber towards QSO SDSS J1143+1420 at z=2.323
errMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
IF4.8
err2022-05-11
err0
errOAAI
errShaw, Gargi; Ranjan, A.
err分享
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Photoionization Modeling of the Dusty Nova V1280 Scorpii
errASTROPHYSICAL JOURNAL
IF5.4
err2022-02-04
err8
errOAAI
errPandey, Ruchi; Das, Ramkrishna; Shaw, Gargi; Mondal, Soumen
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Spectroscopic modelling of two high-mass X-ray binaries, Cyg X-3 and 4U 1538-522
errMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
IF4.8
err2021-08-02
err1
errOAAI
errShaw, Gargi; Bhattacharyya, Sudip
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Role of Polycyclic Aromatic Hydrocarbons on the Cosmic-Ray Ionization Rate in the Galaxy
errASTROPHYSICAL JOURNAL
IF5.4
err2021-02-19
err7
errOAAI
errShaw, Gargi; Ferland, G. J.
err分享
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Physical conditions in two high-redshift H2-bearing GRB-DLAs, 120815A and 121024A
errMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
IF4.8
err2020-03-09
err6
errOAAI
errShaw, Gargi; Ferland, G. J.
err分享
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Spectroscopic modelling of four neutron star low-mass X-ray binaries using CLOUDY
errMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
IF4.8
err2019-03-16
err4
errOAAI
errShaw, Gargi; Bhattacharyya, Sudip
err分享
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A photoionization model grid for novae: estimation of physical parameters
errMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
IF4.8
err2019-01-08
err7
errOAAI
errMondal, Anindita; Das, Ramkrishna; Shaw, Gargi; Mondal, Soumen
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Multicomponent H2 in DLA at zabs=2.05: physical conditions through observations and numerical models
errMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
IF4.8
err2018-08-25
err14
errOAAI
errRawlins, Katherine; Srianand, Raghunathan; Shaw, Gargi; Rahmani, Hadi; Dutta, Rajeshwari; Chacko, Sajeev
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Physical conditions in three high-z H2-bearing DLAs: implications for grain size
errMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
IF4.8
err2016-04-13
err17
errOAAI
errShaw, Gargi; Rawlins, Katherine; Srianand, Raghunathan
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ROVIBRATIONALLY RESOLVED DIRECT PHOTODISSOCIATION THROUGH THE LYMAN AND WERNER TRANSITIONS OF H2 FOR FUV/X-RAY-IRRADIATED ENVIRONMENTS
errASTROPHYSICAL JOURNAL
IF5.4
err2012-01-25
err18
PREAI
errGay, C. D.; Abel, N. P.; Porter, R. L.; Stancil, P. C.; Ferland, G. J.; Shaw, G.; van Hoof, P. A. M.; Williams, R. J. R.
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ORION'S BAR: PHYSICAL CONDITIONS ACROSS THE DEFINITIVE H+/H0/H2 INTERFACE
errASTROPHYSICAL JOURNAL
IF5.4
err2009-03-02
err72
errOAAI
errPellegrini, E. W.; Baldwin, J. A.; Ferland, G. J.; Shaw, G.; Heathcote, S.
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ROTATIONAL QUENCHING RATE COEFFICIENTS FOR H2 IN COLLISIONS WITH H2 FROM 2 TO 10,000 K
errASTROPHYSICAL JOURNAL
IF5.4
err2008-12-20
err31
errOAAI
errLee, T. -G.; Balakrishnan, N.; Forrey, R. C.; Stancil, P. C.; Shaw, G.; Schultz, D. R.; Ferland, G. J.
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ULTRAVIOLET SURVEY OF CO AND H2 IN DIFFUSE MOLECULAR CLOUDS: THE REFLECTION OF TWO PHOTOCHEMISTRY REGIMES IN ABUNDANCE RELATIONSHIPS
errASTROPHYSICAL JOURNAL
IF5.4
err2008-11-10
err239
errOAAI
errSheffer, Y.; Rogers, M.; Federman, S. R.; Abel, N. P.; Gredel, R.; Lambert, D. L.; Shaw, G.
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