Radio Astronomy by Staelin, David H., Rosenkranz, Philip W., Burke, Bernard F., Parrish, Alan, Haschick, Aubrey D., Guiffrida, Thomas S., Walker, Robert C., Baan, Willem A., Crane, Patrick C., Allen, Barry R., Greenfield, Perry E., Garcia-Barreto, J. Antonio, Barrett, John W., Papa, D. Cosmo, Kierstead, John D., Myers, Philip C.

Subjects: “…Microwave Spectroscopy of the Interstellar Medium…”
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Radio Astronomy by Barrett, Alan H., Myers, Philip C., Burke, Bernard F., Shao, Michael, Staelin, David H., Garnavich, Peter M., Lang, Jeffrey H., Johnson, Timothy L., Shih, Shih-Ming, Yam, Yeung, Rosenkranz, Philip W., Komichak, Michael J., Nathan, S. Krishna, Ali, Ali D. S., Ghosh, Biswa, Sulecki, Joan M., Lamb, R. H., Jin, Jian-sheng

Subjects: “…Microwave Spectroscopy of the Interstellar Medium…”
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Radio Astronomy by Barrett, Alan H., Myers, Philip C., Staelin, David H., Rosenkranz, Philip W., Lam, Kai-Shue

Subjects: “…Microwave Spectroscopy of the Interstellar Medium…”
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Radio Astronomy by Shao, Micheal, Staelin, David H., Melcher, James R., Rosenkranz, Philip W., Barrett, Alan H., Myers, Philip C., Burke, Bernard F., Walker, Robert C., Haschick, Aubrey D., Giuffrida, Thomas S., Garcia-Barreto, J. Antonio

Subjects: “…Microwave Spectroscopy of the Interstellar Medium…”
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Radio Astronomy by Barrett, Alan H., Rosenkranz, Philip W., Staelin, David H., Kunzi, Klaus F., Lam, Kai-Shue

Subjects: “…Microwave Spectroscopy of the Interstellar Medium…”
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Radio Astronomy by Barrett, Alan H., Burke, Bernard F., Staelin, David H., Rosenkranz, Philip W., Garnavich, Peter M., Shao, Michael, Colavita, M. Mark, Nathan, Krishna S., Xu, Xi Ru, Troxel, Donald E., Willsky, Alan S., Ali, Ali D. S., Ghosh, Biswa, Lambert, Katherine H., Sulecki, Joan M., Lang, Jeffrey H., Johnson, Timothy L., Yam, Yeung, Shih, Shih-Ming, Karl, William C.

Subjects: “…Microwave Spectroscopy of the Interstellar Medium…”
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Radio Astronomy by Staelin, David H., Shao, Michael, Melcher, James R., Rosenkranz, Philip W., Ledsham, William H., Barrett, Alan H., Myers, Philip C., Walker, Robert C., Burke, Bernard F., Haschick, Aubrey D., Giuffrida, Thomas S., Baan, Willem A.

Subjects: “…Microwave Spectroscopy of the Interstellar Medium…”
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8.282J / 12.402J Introduction to Astronomy, Spring 2003 by Rappaport, S. A., 1942-, Elliot, James, 1943-

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Understanding radio pulsars using modern broad-band instruments by Oswald, LS

“…In order to maximize the understanding available with broad-band observations, it is important to address the interaction between pulsar radio emission and the interstellar medium through which it propagates. I create an algorithm for correcting the effects of the interstellar medium in broad-band polarimetric data from the Parkes Ultra-Wideband receiver to reveal the intrinsic polarization behaviour of PSRs~J1056--6258 and J1359--6038. …”

Magnetic fields and UHECR propagation by Ferrière Katia

“…I review the main observational tools used to detect and measure magnetic fields in the interstellar medium of our Galaxy (considering both the Galactic disk and the Galactic halo), in the interstellar medium of external galaxies, and in the extragalactic medium. …”
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Hot Subdwarf Stars Identified in LAMOST DR8 with Single-lined and Composite Spectra by Zhenxin Lei, Ruijie He, Péter Németh, Joris Vos, Xuan Zou, Ke Hu, Huaping Xiao, Huahui Yan, Jingkun Zhao

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Astrochemistry / by Wilkins, Olivia Harper, author 652629, Blake, Geoffrey A., author 369318, ACS Publications (Online service) 645714

“…From there, the tour visits the interstellar medium, with an emphasis on molecular clouds where stars are born. …”
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Loops and spurs: The angular power spectrum of the Galactic synchrotron background by Mertsch, P, Sarkar, S

“…While previous studies have focussed on either the variation of the emissivity on large (kpc) scales, or on fluctuations due to MHD turbulence in the interstellar medium, we unify these approaches to match the angular power spectrum. …”

Loops and spurs: the angular power spectrum of the Galactic synchrotron background by Mertsch, P, Sarkar, S

“…While previous studies have focussed on either the variation of the emissivity on large (∼ kpc) scales, or on fluctuations due to MHD turbulence in the interstellar medium, we unify these approaches to match the angular power spectrum. …”

Simulating star formation and feedback on a galaxy scale by Slyz, A

“…Insufficient computational power and numerous poorly understood physical processes, force simulations to adopt sub-grid models of the interstellar medium. These may crucially bias results. We advocate for smaller (similar to kiloparsec) scale simulations of the interstellar medium to guide the development of sub-grid models in larger simulations. …”

Searching for an Intermediate Mass Black Hole in the Blue Compact Dwarf galaxy MRK 996 by Georgakakis, A, Tsamis, Y, James, B, Aloisi, A

“…The possibility is explored that accretion on an intermediate mass black hole contributes to the ionisation of the interstellar medium of the Compact Blue Dwarf galaxy MRK996. …”

A polarization census of bright pulsars using the ultrawideband receiver on the Parkes radio telescope by Sobey, C, Johnston, S, Dai, S, Kerr, M, Manchester, RN, Oswald, LS, Parthasarathy, A, Shannon, RM, Weltevrede, P

“…We obtain updated and accurate interstellar medium parameters towards these pulsars (dispersion measures and Faraday rotation measures), and reveal Faraday dispersion towards PSR J1721-3532 caused by interstellar scattering. …”

Mass Distribution for Single-lined Hot Subdwarf Stars in LAMOST by Zhenxin Lei, Ruijie He, Péter Németh, Xuan Zou, Huaping Xiao, Yong Yang, Jingkun Zhao

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Afterglow Light Curves from Off-Axis GRB Jets in Stratified Circumburst Medium by Xiao-Hong Zhao, Kang-Fa Cheng

“…Generally, the afterglow light curves of off-axis GRBs in the homogeneous interstellar medium have a steep rise arising due to jet deceleration. …”
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Contribution of galaxies to the background hydrogen-ionizing flux by Devriendt, J, Sethi, S, Guiderdoni, B, Nath, B

“…We take into account the absorption of Lyman-limit photons by HI and dust in the interstellar medium of the galaxies. We find that the background Lyman-limit flux due to galaxies might dominate (or be comparable to) the contribution from quasars at almost all redshifts if the absorption by HI in the interstellar medium is neglected. …”