2025PASP..137k6001M


Query : 2025PASP..137k6001M

2025PASP..137k6001M - Publ. Astron. Soc. Pac., 137, part no 11, 6001 (2025/November-0)

Radio Stars in the Era of New Observatories.

MATTHEWS L.D.

Abstract (from CDS):

An international conference Radio Stars in the Era of New Observatories was held at the Massachusetts Institute of Technologay Haystack Observatory on 2024 April 17-19. The conference brought together more than 60 researchers from around the world, united by an interest in using radio wavelength observations to explore the physical processes that operate in stars (including the Sun), how stars evolve and interact with their environments, and the role of radio stars as probes of our Galaxy. Topics discussed at the meeting included radio emission from cool and ultracool dwarfs, extrasolar space weather, stellar masers, thermal radio emission from evolved stars, circumstellar chemistry, low frequency observations of the Sun, radio emission from hot stars, applications of very long baseline interferometry techniques to stellar astrophysics, stellar explosive events, the detection of radio stars in the latest generation of widefield sky surveys, the importance of radio stars for understanding the structure and evolution of the Milky Way, and the anticipated applications for stellar astrophysics of future radio observatories on the ground and in space. This article summarizes research topics and results featured at the conference, along with some background and contextual information. It also highlights key outstanding questions in stellar astrophysics where new insights are anticipated from the next generation of observational facilities operating at meter through submillimeter wavelengths.

Abstract Copyright: © 2025. The Astronomical Society of the Pacific. All rights, including for text and data mining, AI training, and similar technologies, are reserved.

Journal keyword(s): Galaxy structure - Astrophysical masers - Radio astronomy - Solar radio emission - Circumstellar envelopes - Stellar activity - Stellar winds - Stellar evolution - Variable stars

Simbad objects: 46

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Number of rows : 46
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 59 EmG 00 15 25.126 -21 26 39.68 14.01 13.21 12.59 12.31   ~ 111 0
2 LP 349-25 SB* 00 27 56.0057038615 +22 19 32.635434516   18.6   16.0   M8Ve 82 0
3 V* YZ Cet PM* 01 12 30.6368826382 -16 59 56.358011559 15.315 13.885 12.074 10.696 8.938 M4.0Ve 335 0
4 V* R Scl C* 01 26 58.0939182720 -32 32 35.439234828 17.26 9.59 5.72 3.69 2.30 C-N5+ 354 0
5 * omi Cet Mi* 02 19 20.79210 -02 58 39.4956   7.63 6.53 5.03   M5-9IIIe+DA 1586 0
6 HD 22468 RS* 03 36 47.2904292073 +00 35 15.943692002 7.09 6.79 5.90     K2:Vnk 1206 0
7 V* IK Tau OH* 03 53 28.8924743304 +11 24 21.895183368 16.99 14.463 16.171 14.101   M7-11 675 0
8 TMC-1 MoC 04 41 45.9 +25 41 27           ~ 1872 0
9 V* R Lep C* 04 59 36.3486921120 -14 48 22.502479140 15.06 13.51 7.76 4.90 3.42 C7,6e 360 0
10 V* AB Dor TT* 05 28 44.8712165880 -65 26 55.199147208 8.259 7.856 6.999 6.496 5.993 K0V 1080 0
11 NAME Orion Nebula Cluster OpC 05 35.0 -05 29           ~ 2514 0
12 [RLK73] IRc 2 IR 05 35 14.51548 -05 22 30.5943           ~ 673 1
13 IRC +70066 Mi* 05 46 44.3288397432 +69 58 24.422766636           M9.5 94 0
14 * alf Ori s*r 05 55 10.30536 +07 24 25.4304 4.38 2.27 0.42 -1.17 -2.45 M1-M2Ia-Iab 1789 0
15 WISEP J062309.94-045624.6 BD* 06 23 09.682704 -04 56 23.52372           T8 19 0
16 PN Vo 1 PN 06 59 26.4167860656 -79 38 47.118534828           [WC10] 111 0
17 V* VY CMa s*r 07 22 58.3261352189 -25 46 03.194390594 12.01 10.068 8.691 7.938   M5Iae 1169 0
18 IRC +10216 C* 09 47 57.40632 +13 16 43.5648           C9,5e 2455 0
19 2MASS J10190575+6529526 BD* 10 19 05.75424 +65 29 52.6956           T6 13 0
20 2MASS J11225550+2550250 BD* 11 22 55.50384 +25 50 25.0728           T6 33 0
21 V* V357 Mus No* 11 26 15.160 -65 31 23.30           ~ 32 0
22 V* R Hya Mi* 13 29 42.7801586466 -23 16 52.751628992 7.26 6.58 4.97 2.27 -0.15 M6-9e 511 0
23 V* DG CVn ** 13 31 46.6246175093 +29 16 36.681048898   12.90 12.02 10.77 9.15 M4Ve 135 0
24 V* W Hya Mi* 13 49 02.0018313132 -28 22 03.532006894   8.97 7.70     M7.5-9e 672 0
25 V* CU Vir a2* 14 12 15.8055434051 +02 24 33.945178515 4.46 4.90 5.02 5.10 5.23 ApSi 411 0
26 TVLM 513-46 BD* 15 01 08.1864639648 +22 50 02.137869060   21.4 15.09 18.0   M8.5V 189 0
27 V* HR Lup a2* 15 08 12.1238757000 -40 35 02.155417224 5.25 5.65 5.79     B8IVSi 186 1
28 V* AR Sco EB* 16 21 47.2831986456 -22 53 10.385689092   14.94 14.75     M5+D? 141 0
29 GSS 35 TT* 16 26 34.1761719864 -24 23 28.283473860     16.53 14.75 12.51 B3 254 1
30 NAME Ophiuchus Molecular Cloud SFR 16 28 06 -24 32.5           ~ 3969 1
31 V* AH Sco s*r 17 11 17.0194487616 -32 19 30.714035556   10.03 8.10     M5Ia-Iab 145 0
32 NGC 6334A HII 17 20 19.3 -35 54 55           ~ 123 0
33 [BHT2019] G358.93-00.03 MM1 mm 17 43 10.1014 -29 51 45.693           ~ 37 0
34 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
35 V* V1324 Sco No* 17 50 53.9093841216 -32 37 21.090962028           ~ 100 0
36 V* V745 Sco Sy* 17 55 22.2260994408 -33 14 58.551839808     17.987   13.353 M2/M6IIIe 265 1
37 IRAS 18043-2116 OH* 18 07 20.86584 -21 16 12.1116           O-rich 45 0
38 V* VX Sgr s*r 18 08 04.0442790744 -22 13 26.600899044 11.72 9.41 6.52 3.90 2.11 M8.5Ia 622 0
39 NAME Serpens Cloud SFR 18 29 49 +01 14.8           ~ 1195 1
40 [EC92] 95 Y*O 18 29 57.893 +01 12 46.25           K1.0 79 3
41 LSR J1835+3259 PM* 18 35 37.8801226673 +32 59 53.316099140   20.0   17.1   M8.5V 160 0
42 OH 031.0-00.2 OH* 18 48 43.01976 -01 48 30.1464           O-rich 57 0
43 NOVA Her 2021 No* 18 57 30.9832440660 +16 53 39.589542422           ~ 79 0
44 NGC 7000 Cl* 20 58 47 +44 19.8           ~ 427 0
45 * pi.01 Gru S* 22 22 44.2083897000 -45 56 52.791160956 10.52 8.62 6.55 3.19 0.52 S5,7: 216 0
46 BD+19 5116 ** 23 31 52.17898 +19 56 14.1505 12.737 11.749 10.165 8.982 7.446 M3.5V 469 0

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