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1by Kirk, H., Dunham, M. M., Francesco, J. Di, Johnstone, D., Offner, S. S. R., Sadavoy, S. I., Tobin, J. J., Arce, H. G., Bourke, T. L., Mairs, S., Myers, P. C., Pineda, J. E., Schnee, S., Shirley, Y. L.“... '' from the nearest Spitzer young stellar object. Only one of these has strong evidence for being truly...”
Published 2017
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2by Bieging, John H., Patel, Saahil, Peters, William L., Toth, L. Viktor, Marton, Gábor, Zahorecz, Sarolta“... that the young stellar object surface density scales as approximately the 1.6-power of the gas column density...”
Published 2016
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3by Watson, Dan M., Calvet, Nuria P., Fischer, William J., Forrest, W. J., Manoj, P., Megeath, S. Thomas, Melnick, Gary J., Najita, Joan, Neufeld, David A., Sheehan, Patrick D., Stutz, Amelia M., Tobin, John J.“...), which continues through the Class 0 range the trend observed in Class II young stellar objects. Along...”
Published 2016
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4by Zasowski, G., Cohen, R. E., Chojnowski, S. D., Santana, F., Oelkers, R. J., Andrews, B., Beaton, R. L., Bender, C., Bird, J. C., Bovy, J., Carlberg, J. K., Covey, K., Cunha, K., Dell’Agli, F., Fleming, Scott W., Frinchaboy, P. M., García-Hernández, D. A., Harding, P., Holtzman, J., Johnson, J. A., Kollmeier, J. A., Majewski, S. R., Mészáros, Sz., Munn, J., Muñoz, R. R., Ness, M. K., Nidever, D. L., Poleski, R., Román-Zúñiga, C., Shetrone, M., Simon, J. D., Smith, V. V., Sobeck, J. S., Stringfellow, G. S., Szigetiáros, L., Tayar, J., Troup, N.“... giant branch and red clump stars, RR Lyrae, lowmass dwarf stars, young stellar objects, and numerous...”
Published 2017
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5“... and 109 arcmin(2) at 6 cm, containing 778 near-infrared detected young stellar objects and 190 Hubble...”
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6by Jose, Jessy, Kim, Jinyoung S., Herczeg, Gregory J., Samal, Manash R., Bieging, John H., Meyer, Michael R., Sherry, William H.“... photometry. Based on the infrared excess, we identify 812 candidate young stellar objects (YSOs...”
Published 2016
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7by Bond, Howard E., Ciardullo, Robin, Esplin, Taran L., Hawley, Steven A., Liebert, James, Munari, Ulisse“... SED is very similar to that of Class 0/I young stellar objects. We suggest a scenario in which the EGB...”
Published 2016
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