Search Results - Pinto, C.

Diagnosing the accretion flow in ultraluminous X-ray sources using soft X-ray atomic features by Middleton, M., Walton, D., Fabian, A., Roberts, T., Heil, L., Pinto, C., Anderson, Gemma, Sutton, A.

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From ultraluminous X-ray sources to ultraluminous supersoft sources: NGC 55 ULX, the missing link by Pinto, C., Alston, W., Soria, Roberto, Middleton, M., Walton, D., Sutton, A., Fabian, A., Earnshaw, H., Urquhart, Ryan, Kara, E., Roberts, T.

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HST imaging of the dusty filaments and nucleus swirl in NGC4696 at the centre of the Centaurus Cluster by Fabian, A.C., Walker, S.A., Russell, H.R., Pinto, C., Canning, R.E.A., Salome, P., Sanders, J.S., Taylor, G.B., Zweibel, E.G., Conselice, Christopher J., Combes, F., Crawford, C.S., Ferland, G.J., Gallager, J.S., Hatch, Nina A., Johnstone, R.M., Reynolds, C.S.

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NuSTAR reveals the hidden nature of SS433 by Middleton, M.J., Walton, D.J., Alston, W., Dauser, T., Eikenberry, S., Jiang, Y.F., Fabian, A.C., Fuerst, F., Brightman, M., Marshall, H., Parker, M., Pinto, C., Harrison, F.A., Bachetti, M., Altamirano, D., Bird, A.J., Perez, G., Miller-Jones, James, Charles, P., Boggs, S., Christensen, F., Craig, W., Forster, K., Grefenstette, B., Hailey, C., Madsen, K., Stern, D., Zhang, W.

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