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Items: 1 to 20 of 87

1.

Asteroseismology. Echography of young stars reveals their evolution.

Zwintz K, Fossati L, Ryabchikova T, Guenther D, Aerts C, Barnes TG, Themeßl N, Lorenz D, Cameron C, Kuschnig R, Pollack-Drs S, Moravveji E, Baglin A, Matthews JM, Moffat AF, Poretti E, Rainer M, Rucinski SM, Sasselov D, Weiss WW.

Science. 2014 Aug 1;345(6196):550-3. doi: 10.1126/science.1253645. Epub 2014 Jul 3.

2.

The formation of a massive protostar through the disk accretion of gas.

Chini R, Hoffmeister V, Kimeswenger S, Nielbock M, Nürnberger D, Schmidtobreick L, Sterzik M.

Nature. 2004 May 13;429(6988):155-7.

PMID:
15141204
3.

The formation of stars by gravitational collapse rather than competitive accretion.

Krumholz MR, McKee CF, Klein RI.

Nature. 2005 Nov 17;438(7066):332-4.

PMID:
16292305
4.

Pre-Main-Sequence Star Candidates in the Bar of the Large Magellanic Cloud

Beaulieu JP, Lamers HJGLM, Grison P, Julien R, Lanciaux C, Ferlet R, Vidal-Madjar A, Bertin E, Maurice E, Prevot L, Gry C, Guibert J, Moreau O, Tajhmady F, Aubourg E, Bareyre P, de Kat J, Gros M, Laurent B, Lachieze-Rey M, Lesquoy E, Magneville C, Milsztajn A, Moscoso L, Queinnec F, Renault C, Rich J, Spiro M, Vigroux L, Zylberajch S, Ansari R, Cavalier F, Moniez M.

Science. 1996 May 17;272(5264):995-7.

PMID:
8662586
5.

Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars.

Bedding TR, Mosser B, Huber D, Montalbán J, Beck P, Christensen-Dalsgaard J, Elsworth YP, García RA, Miglio A, Stello D, White TR, De Ridder J, Hekker S, Aerts C, Barban C, Belkacem K, Broomhall AM, Brown TM, Buzasi DL, Carrier F, Chaplin WJ, Di Mauro MP, Dupret MA, Frandsen S, Gilliland RL, Goupil MJ, Jenkins JM, Kallinger T, Kawaler S, Kjeldsen H, Mathur S, Noels A, Aguirre VS, Ventura P.

Nature. 2011 Mar 31;471(7340):608-11. doi: 10.1038/nature09935.

PMID:
21455175
6.

Sodium content as a predictor of the advanced evolution of globular cluster stars.

Campbell SW, D'Orazi V, Yong D, Constantino TN, Lattanzio JC, Stancliffe RJ, Angelou GC, Wylie-de Boer EC, Grundahl F.

Nature. 2013 Jun 13;498(7453):198-200. doi: 10.1038/nature12191. Epub 2013 May 29.

PMID:
23719375
7.

[Molecular spectral diagnosis of star forming regions].

Xi S, Qin S, Deng L, Yang J.

Guang Pu Xue Yu Guang Pu Fen Xi. 2001 Aug;21(4):456-8. Chinese.

PMID:
12945260
8.

Star Formation in W49A: Gravitational Collapse of the Molecular Cloud Core Toward a Ring of Massive Stars.

Welch WJ, Dreher JW, Jackson JM, Terebey S, Vogel SN.

Science. 1987 Dec 11;238(4833):1550-5.

PMID:
17784292
9.

Weakened magnetic braking as the origin of anomalously rapid rotation in old field stars.

van Saders JL, Ceillier T, Metcalfe TS, Aguirre VS, Pinsonneault MH, García RA, Mathur S, Davies GR.

Nature. 2016 Jan 14;529(7585):181-4. doi: 10.1038/nature16168. Epub 2016 Jan 4.

PMID:
26727162
10.

Low-mass relics of early star formation.

Schneider R, Ferrara A, Salvaterra R, Omukai K, Bromm V.

Nature. 2003 Apr 24;422(6934):869-71.

PMID:
12712198
11.

A minimum column density of 1 g cm(-2) for massive star formation.

Krumholz MR, McKee CF.

Nature. 2008 Feb 28;451(7182):1082-4. doi: 10.1038/nature06620.

PMID:
18305539
12.

Gravitationally redshifted absorption lines in the X-ray burst spectra of a neutron star.

Cottam J, Paerels F, Mendez M.

Nature. 2002 Nov 7;420(6911):51-4.

PMID:
12422210
13.
14.

Surprising dissimilarities in a newly formed pair of 'identical twin' stars.

Stassun KG, Mathieu RD, Cargile PA, Aarnio AN, Stempels E, Geller A.

Nature. 2008 Jun 19;453(7198):1079-82. doi: 10.1038/nature07069.

PMID:
18563159
15.

Pulsed accretion in a variable protostar.

Muzerolle J, Furlan E, Flaherty K, Balog Z, Gutermuth R.

Nature. 2013 Jan 17;493(7432):378-80. doi: 10.1038/nature11746. Epub 2013 Jan 2.

PMID:
23283175
16.

The formation of the first star in the Universe.

Abel T, Bryan GL, Norman ML.

Science. 2002 Jan 4;295(5552):93-8. Epub 2001 Nov 15.

17.

Infall of gas as the formation mechanism of stars up to 20 times more massive than the Sun.

Beltrán MT, Cesaroni R, Codella C, Testi L, Furuya RS, Olmi L.

Nature. 2006 Sep 28;443(7110):427-9.

PMID:
17006508
18.

The origin of OB runaway stars.

Fujii MS, Portegies Zwart S.

Science. 2011 Dec 9;334(6061):1380-3. doi: 10.1126/science.1211927. Epub 2011 Nov 17.

19.

Asteroseismology can reveal strong internal magnetic fields in red giant stars.

Fuller J, Cantiello M, Stello D, Garcia RA, Bildsten L.

Science. 2015 Oct 23;350(6259):423-6. doi: 10.1126/science.aac6933.

20.

Seismic evidence for the loss of stellar angular momentum before the white-dwarf stage.

Charpinet S, Fontaine G, Brassard P.

Nature. 2009 Sep 24;461(7263):501-3. doi: 10.1038/nature08307.

PMID:
19779446

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