Results 231 to 240 of about 10,060 (266)

A first look at rocky exoplanets with JWST. [PDF]

Proc Natl Acad Sci U S A
Kreidberg L, Stevenson KB.
europepmc   +1 more source

Extreme properties of a compact and massive accreting black hole host in the first 500 Myr. [PDF]

Nat Commun
Tripodi R, Martis N, Markov V, Bradač M, Di Mascia F, Cammelli V, D'Eugenio F, Willott C, Curti M, Bhatt M, Gallerani S, Rihtaršič G, Singh J, Gaspar G, Harshan A, Judež J, Merida RM, Desprez G, Sawicki M, Goovaerts I, Muzzin A, Noirot G, Sarrouh GTE, Abraham R, Asada Y, Brammer G, Estrada-Carpenter V, Felicioni G, Fujimoto S, Iyer K, Mowla L, Strait V.   +31 more
europepmc   +1 more source

Polarimetry of Early Emission Line Stars.

, 2001
openaire   +1 more source

Magnetic star-planet interaction in the young exoplanet system DS Tucanae Ab

Santos Ld, Owen J, Duvvuri G, Loyd ROP, Vidotto A, Presa A, Bourrier V, King G, Airapetian V, Ehrenreich D, France K, Lendl M, Lothringer J, Nielsen L.   +13 more
europepmc   +1 more source

Early-type emission-line stars

openaire   +1 more source

The Astrophysics of Emission-Line Stars [PDF]

Astrophysics and Space Science Library, 2007
Tomokazu Kogure
exaly   +2 more sources

A photometric catalogue of southern emission-line stars *,** [PDF]

Astronomy and Astrophysics, 2001
We present a catalogue of previously unpublished optical and infrared photometry for a sample of 162 emission-line objects and shell stars visible from the southern hemisphere. The data were obtained between 1978 and 1997 in the Walraven (WULBV), Johnson/Cousins (UBV(RI)_c) and ESO and SAAO near-infrared (JHKLM) photometric systems.
C Eiroa, F J Molster, D de Winter
exaly   +3 more sources

Some of the next articles are maybe not open access.

Related searches:

A survey of emission-line stars in the CMa star formation region

Astrophysics and Space Science, 1986
A survey of emission-line stars was carried out in the CMa star formation region, based on spectral observations with the Kiso Schmidt telescope. In total, 128 emission-line stars were detected, ranging from V = 6 to 15, and the majority are found with V between 11 and 14.
Suhardja D. Wiramihardja, Tomokazu Kogure, Makoto Nakano, Shigeomi Yoshida, Ken’ichi Tatematsu   +4 more
openaire   +1 more source

Emission-line Central Stars of Planetary Nebulae

AIP Conference Proceedings, 2005
The temperatures of central stars of planetary nebulae (PNe) are compared with evolutionary tracks. © 2005 American Institute of Physics.
Gesicki, K., Zijlstra, A. A.; id_orcid 0000-0002-3171-5469, Acker, A.   +2 more
openaire   +2 more sources