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1. The first galaxies in the universe
by Loeb, Abraham
2013, STU - Student edition, Princeton Series in Astrophysics, ISBN 0691144923, cm.
This book provides a comprehensive, self-contained introduction to one of the most exciting frontiers in astrophysics today: the quest to understand how the... 
Galaxies | Physics | PHVB | Astrophysics | PGK | PGM | Science | Cosmology | Space Science | Stars | General Science | Formation | Astronomy
Book
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2. The formation of stars
by Stahler, Steven William
2004, ISBN 3527405593, xiii, 852
Book
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3. Full Text The formation and destruction of molecular clouds and galactic star formation: An origin for the cloud mass function and star formation efficiency
by Inutsuka, Shu-Ichiro and Inoue, Tsuyoshi and Iwasaki, Kazunari and Hosokawa, Takashi
Astronomy and Astrophysics, ISSN 0004-6361, 08/2015, Volume 580, p. A49
We describe an overall picture of galactic-scale star formation. Recent high-resolution magneto-hydrodynamical simulations of two-fluid dynamics with cooling,... 
ISM: clouds | Stars: formation | ISM: bubbles | ISM: structure | ISM: kinematics and dynamics | ISM: magnetic fields | GAS DEPLETION TIME | MAGNETOHYDRODYNAMIC SIMULATIONS | DISSOCIATION FRONT | FORMATION RATES | DYNAMICAL EXPANSION | stars: formation | GSH 277+00+36 | H I FLOWS | ASTRONOMY & ASTROPHYSICS | MAGNETIC-FIELD | LARGE-MAGELLANIC-CLOUD | ACCRETION FLOWS | Clouds | Destruction | Exponents | Star formation | Simulation | Molecular clouds | Time | Formations
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4. The formation of the solar system
: theories old and new
by Woolfson, Michael M. author. (Michael Mark)
2015, 2nd edition., ISBN 1783265213, xxii, 418 pages
Solar system Origin
Book
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5. Full Text Characterization of exoplanets from their formation: I. Models of combined planet formation and evolution
by Mordasini, C and Alibert, Y and Klahr, H and Henning, T
Astronomy and Astrophysics, ISSN 0004-6361, 2012, Volume 547, p. A111
Context. A first characterization of extrasolar planets by the observational determination of the radius has recently been achieved for a large number of... 
Planets and satellites: interiors | Planet-disk interactions | Planets and satellites: individual: Jupiter | Planets and satellites: formation | Methods: numerical | Planetary systems | EXTRASOLAR GIANT PLANETS | planets and satellites: interiors | PROTOPLANETARY DISKS | GRAVITATIONAL-INSTABILITY | LOW-MASS STARS | GASEOUS ENVELOPE | YOUNG JUPITERS | methods: numerical | planets and satellites: individual: Jupiter | planetary systems | BROWN DWARFS | GAS ACCRETION | ASTRONOMY & ASTROPHYSICS | planet-disk interactions | DISK ACCRETION | planets and satellites: formation | HR 8799 | Physics - Earth and Planetary Astrophysics
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6. Full Text Fragmentation and disk formation during high-mass star formation: IRAM NOEMA (Northern Extended Millimeter Array) large program CORE
by Beuther, H and Mottram, J.C and Ahmadi, A and Bosco, F and Linz, H and Henning, T and Klaassen, P and Winters, J.M and Maud, L.T and Kuiper, R and Semenov, D and Gieser, C and Peters, T and Urquhart, J.S and Pudritz, R and Ragan, S.E and Feng, S and Keto, E and Leurini, S and Cesaroni, R and Beltran, M and Palau, A and Sánchez-Monge, A and Galvan-Madrid, R and Zhang, Q and Schilke, P and Wyrowski, F and Johnston, K.G and Longmore, S.N and Lumsden, S and Hoare, M and Menten, K.M and Csengeri, T
Astronomy and Astrophysics, ISSN 0004-6361, 09/2018, Volume 617, p. A100
Context. High-mass stars form in clusters, but neither the early fragmentation processes nor the detailed physical processes leading to the most massive stars... 
Stars: formation | Stars: general | Instrumentation: interferometers | Stars: massive | Stars: rotation | DUST CONTINUUM | PHYSICAL CONDITIONS | stars: general | CONTINUUM EMISSION | SAMPLE | stars: formation | EVOLUTION | ASTRONOMY & ASTROPHYSICS | PROTOSTARS | stars: massive | PROTOSTELLAR CANDIDATES | ACCRETION | stars: rotation | instrumentation: interferometers | HII-REGIONS | TRIGONOMETRIC PARALLAXES
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7. FORMATION OF THE SOLAR SYSTEM: THEORIES OLD AND NEW
by WOOLFSON, MICHAEL
2007, ISBN 1860948243
Book
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8. How did the first stars and galaxies form?
by Loeb, Abraham
2010, STU - Student edition, Princeton frontiers in physics, ISBN 9780691145150, xiii, 193
Though astrophysicists have developed a theoretical framework for understanding how the first stars and galaxies formed, only now are we able to begin testing... 
Cosmology | Galaxies | Formation | Stars | Physics | Science | Astronomy- Science | Astrophysics- PGM- PHVB | Astronomy
Book
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9. Full Text On Star Formation Rates and Star Formation Histories of Galaxies Out to z ~ 3
by Wuyts, Stijn and Förster Schreiber, Natascha M and Lutz, Dieter and Nordon, Raanan and Berta, Stefano and Altieri, Bruno and Andreani, Paola and Aussel, Hervé and Bongiovanni, Angel and Cepa, Jordi and Cimatti, Andrea and Daddi, Emanuele and Elbaz, David and Genzel, Reinhard and Koekemoer, Anton M and Magnelli, Benjamin and Maiolino, Roberto and McGrath, Elizabeth J and García, Ana Pérez and Poglitsch, Albrecht and Popesso, Paola and Pozzi, Francesca and Sanchez-Portal, Miguel and Sturm, Eckhard and Tacconi, Linda and Valtchanov, Ivan
The Astrophysical Journal, ISSN 0004-637X, 09/2011, Volume 738, Issue 1, p. 106
We compare multi-wavelength SFR indicators out to z~3 in GOODS-South. Our analysis uniquely combines U-to-8um photometry from FIREWORKS, MIPS 24um and PACS 70,... 
galaxies: high-redshift | galaxies: stellar content | Physics - Cosmology and Nongalactic Astrophysics | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | PHOTOMETRY | ENERGY SPECTRA | STARS | GALAXIES | SIMULATION | SPECTRA
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10. Full Text THE BURSTY STAR FORMATION HISTORIES of LOW-MASS GALAXIES at 0.4 < z < 1 REVEALED by STAR FORMATION RATES MEASURED from Hβ and FUV
by Guo, Yicheng and Rafelski, Marc and Faber, S.M and Koo, David C and Krumholz, Mark R and Trump, Jonathan R and Willner, S.P and Amorín, Ricardo and Barro, Guillermo and Bell, Eric F and Gardner, Jonathan P and Gawiser, Eric and Hathi, Nimish P and Koekemoer, Anton M and Pacifici, Camilla and Pérez-González, Pablo G and Ravindranath, Swara and Reddy, Naveen and Teplitz, Harry I and Yesuf, Hassen
Astrophysical Journal, ISSN 0004-637X, 12/2016, Volume 833, Issue 1
We investigate the burstiness of star formation histories (SFHs) of galaxies at 0.4 < z < 1 by using the ratio of star formation rates (SFRs) measured from H... 
galaxies: dwarf | galaxies: formation | galaxies: fundamental parameters | galaxies: starburst | galaxies: evolution | galaxies: star formation | CONTINUUM ESCAPE FRACTION | FORMATION RATE INDICATORS | LESS-THAN 1.5 | HUBBLE-SPACE-TELESCOPE | SIMILAR-TO 2 | GOODS-SOUTH FIELD | EXTRAGALACTIC LEGACY SURVEY | ASTRONOMY & ASTROPHYSICS | DUST ATTENUATION CURVE | LARGE-MAGELLANIC-CLOUD | STELLAR POPULATION SYNTHESIS | Physics - Astrophysics of Galaxies | CORRECTIONS | TELESCOPES | RED SHIFT | STOCHASTIC PROCESSES | SPACE | STAR CLUSTERS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | STAR EVOLUTION | IMAGES | ATTENUATION | MASS | STARS | MILKY WAY | FAR ULTRAVIOLET RADIATION | COSMIC DUST
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11. Full Text Molecular cloud formation and the star formation efficiency in M 33: Molecule and star formation in M 33
by Braine, J and Gratier, P and Kramer, C and Schuster, K.F and Tabatabaei, F and Gardan, E
Astronomy and Astrophysics, ISSN 0004-6361, 10/2010, Volume 520, Issue 15, p. A107
Does star formation proceed in the same way in large spirals such as the Milky Way and in smaller chemically younger galaxies? Earlier work suggests a more... 
stars: formation | ISM: clouds | Local Group | galaxies: groups: individual: M 33 | galaxies: evolution | galaxies: ISM | MAGELLANIC-CLOUD | OUTER GALAXY | METALLICITY | M33 | ISOLATED SPIRAL GALAXY | CARBON-MONOXIDE | ASTRONOMY & ASTROPHYSICS | GAS | (CO)-C-13 | EMISSION | Solar and Stellar Astrophysics | Sciences of the Universe | Astrophysics | Physics
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12. Full Text Probing the initial conditions of high-mass star formation III. Fragmentation and triggered star formation
by Zhang, CP and Csengeri, T and Wyrowski, F and Li, GX and Pillai, T and Menten, KM and Hatchell, J and Thompson, MA and Pestalozzi, MR
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 07/2019, Volume 627, p. A85
Context. Fragmentation and feedback are two important processes during the early phases of star formation. Aims. Massive clumps tend to fragment into clusters... 
methods: observational | STELLAR CLUSTERS | GRAVITATIONAL COLLAPSE | RESOLUTION | FORMING REGIONS | TURBULENT | RADIATION | stars: formation | ASTRONOMY & ASTROPHYSICS | DYNAMICS | ACCRETION | ISM: clouds | METHANOL MASERS | techniques: interferometric | TRIGONOMETRIC PARALLAXES
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13. Full Text An uncertainty principle for star formation - I. why galactic star formation relations break down below a certain spatial scale
by Diederik Kruijssen, J.M and Longmore, Steven N
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2014, Volume 439, Issue 4, pp. 3239 - 3252
Galactic scaling relations between the (surface densities of) the gas mass and the star formation (SF) rate are known to develop substantial scatter or even... 
Galaxies: stellar content | Galaxies: evolution | ISM: evolution | Stars: formation | Galaxies: ISM | GAS DEPLETION TIME | FORMATION LAW | MOLECULAR CLOUDS | galaxies: evolution | KPC SCALES | NGC 5194 | YOUNG STELLAR OBJECTS | stars: formation | galaxies: ISM | ASTRONOMY & ASTROPHYSICS | INITIAL MASS FUNCTION | MILKY-WAY | galaxies: stellar content | SCHMIDT LAW | NEARBY DISK GALAXIES
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14. The interstellar medium, expanding nebulae and triggered star formation
: theory and simulations
by Bisbas, Thomas G. author
2016, SpringerBriefs in Astronomy, ISBN 9783319261409, xi, 71 pages
This brief brings together the theoretical aspects of star formation and ionized regions with the most up-to-date simulations and observations. Beginning with... 
Nebulae | Interstellar matter | Astrophysics
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15. Full Text Cosmic star-formation history
by Madau, Piero and Dickinson, Mark
Annual Review of Astronomy and Astrophysics, ISSN 0066-4146, 2014, Volume 52, Issue 1, pp. 415 - 486
Over the past two decades, an avalanche of new data from multiwavelength imaging and spectroscopic surveys has revolutionized our view of galaxy formation and... 
galaxy formation | star formation | cosmology | evolution | stellar populations | LYMAN-BREAK GALAXIES | SIMILAR-TO 2 | HUBBLE-DEEP-FIELD | HIGH-REDSHIFT GALAXIES | ULTRAVIOLET LUMINOSITY DENSITY | SPECTRAL ENERGY-DISTRIBUTIONS | EXTRAGALACTIC LEGACY SURVEY | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | STELLAR MASS FUNCTION | REST-FRAME ULTRAVIOLET | Star formation | Observations | Physics - Cosmology and Nongalactic Astrophysics
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